This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ
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 08.4224 2461321.9224 12.51 09:56:37.44 +18:09:06.6
216.06818 48.88848 galactic Leo Second-epoch detections are separated by 1.7" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.196 Philomela -0 -0 0 12.9 0 0
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits at 09:56:37.44 +18:09:06.6: 15.95 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits at 09:56:37.44 +18:09:06.6: 16.03 +/- 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 08.4224* 09 56 37.44 +18 09 06.6 12.5 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,2461321.9224,12.51,0.05,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 20261008.4224 12.51CV 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 08.4224 2461321.9224 12.77 09:37:32.57 +21:23:11.2
209.39762 45.69882 galactic Leo Second-epoch detections are separated by 1.5" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.68 Leto 0 -0 0 13.0 0 0
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits at 09:37:32.57 +21:23:11.2: 15.77 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits at 09:37:32.57 +21:23:11.2: 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 08.4224* 09 37 32.57 +21 23 11.2 12.8 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,2461321.9224,12.77,0.05,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 20261008.4224 12.77CV 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 08.4224 2461321.9224 12.46 10:26:19.69 +20:20:32.0
216.57125 56.22627 galactic Leo Second-epoch detections are separated by 0.9" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.471 Papagena -0 -0 0 12.1 0 -0
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits at 10:26:19.69 +20:20:32.0: 15.90 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits at 10:26:19.69 +20:20:32.0: 15.90 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 08.4224* 10 26 19.69 +20 20 32.0 12.5 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,2461321.9224,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261008.4224 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 08.4224 2461321.9224 13.46 09:54:49.47 +19:24:25.6
214.05205 48.91879 galactic Leo Second-epoch detections are separated by 0.9" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J148.7061+19.4072 | 09:54:49.47 +19:24:25.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.820+/-0.027 (M)
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits at 09:54:49.47 +19:24:25.6: 16.00 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits at 09:54:49.47 +19:24:25.6: 16.02 +/- 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 08.4224* 09 54 49.47 +19 24 25.6 13.5 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
ATO J148.7061+19.4072,2461321.9224,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J148.7061+19.4072 20261008.4224 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 08.4224 2461321.9224 13.44 09:42:41.53 +18:01:29.9
214.51626 45.74656 galactic Leo Second-epoch detections are separated by 0.7" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.245 Vera 0 0 0 13.9 -0 0
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits at 09:42:41.53 +18:01:29.9: 15.77 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits at 09:42:41.53 +18:01:29.9: 15.81 +/- 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 08.4224* 09 42 41.53 +18 01 29.9 13.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461321.9224,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261008.4224 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 08.4224 2461321.9224 13.52 09:42:15.69 +22:07:08.8
208.84791 46.96103 galactic Leo Second-epoch detections are separated by 0.7" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.87 Sylvia -0 -0 1 13.7 0 -0
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits at 09:42:15.69 +22:07:08.8: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits at 09:42:15.69 +22:07:08.8: 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 08.4224* 09 42 15.69 +22 07 08.8 13.5 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,2461321.9224,13.52,0.05,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 20261008.4224 13.52CV 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 08.4224 2461321.9224 13.73 09:53:45.36 +19:33:59.9
213.69704 48.73375 galactic Leo Second-epoch detections are separated by 1.8" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.134 Sophrosyne -0 -0 0 14.1 0 0
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits at 09:53:45.36 +19:33:59.9: 15.95 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits at 09:53:45.36 +19:33:59.9: 15.94 +/- 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 08.4224* 09 53 45.36 +19 33 59.9 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,2461321.9224,13.73,0.05,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 20261008.4224 13.73CV 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 08.4224 2461321.9224 14.13 09:58:58.79 +17:10:02.5
217.77601 49.05386 galactic Leo Second-epoch detections are separated by 2.6" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.209 Dido 2 -0 2 14.5 -0 0
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits at 09:58:58.79 +17:10:02.5: 15.90 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits at 09:58:58.79 +17:10:02.5: 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 08.4224* 09 58 58.79 +17 10 02.5 14.1 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,2461321.9224,14.13,0.05,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 20261008.4224 14.13CV 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: 2461139.72915330 09.04.2026 05:29:48.845 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits
First image: 2461139.72915330 09.04.2026 05:29:48.845 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits
Last image: 2461321.92282529 08.10.2026 10:08:42.105 /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.28
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 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): 6215
Objects passed selection criteria: 6200
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 4979.25
Average stars matched: 4855 (97.5046 %)
Memory usage VmPeak: 239536 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Oct 6 12:01:37 CDT 2026
VaST build number 1.0rc89-233-gd5bdb823
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-06)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Oct 8 05:12:42 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: 2461139.72915330 09.04.2026 05:29:48.845 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits
First image: 2461139.72915330 09.04.2026 05:29:48.845 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits
Last image: 2461321.92282529 08.10.2026 10:08:42.105 /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 32
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.03
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: 12 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): 31423
Objects passed selection criteria: 31349
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: 27315.2
Average stars matched: 26153.2 (95.746 %)
Memory usage VmPeak: 258968 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Oct 6 12:01:37 CDT 2026
VaST build number 1.0rc89-233-gd5bdb823
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-06)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Oct 8 05:13:31 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-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits
SExtractor catalog cache: saved Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits.cat to cache
SExtractor catalog cache: saved Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.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-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.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: 2461321.92204773
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-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits exists and is non-empty
wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits exists and is non-empty
wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits exists and is non-empty
wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits (1st reference image)
verification OK: wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits
Image size: 937.4'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: 10:09:13.907 +22:00:17.19 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-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits (1st new image)
verification OK: wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits
Image size: 945.2'x627.0' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 10:09:07.439 +21:56:58.14 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 10:09:13.907 +22:00:17.19
Second-epoch image center 10:09:07.439 +21:56:58.14
Angular distance between the image centers 0.0607 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits (2nd new image)
verification OK: wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits
Image size: 945.0'x627.0' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 10:09:08.624 +21:57:32.16 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 10:09:13.907 +22:00:17.19
Second-epoch image center 10:09:08.624 +21:57:32.16
Angular distance between the image centers 0.0502 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 10:09:07.439 +21:56:58.14
Second-epoch second image center 10:09:08.624 +21:57:32.16
Angular distance between the image centers 0.01050 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-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits &> /tmp/tmp.NctIo1WiRn
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits &> /tmp/tmp.JFSHAdS7FC
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits &> /tmp/tmp.5zKJfqSltk
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits &> /tmp/tmp.S3CGH0qGyp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.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-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits and wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.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-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits and wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits.wcscat
Found non-empty wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits and wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits.wcscat
The reference image (wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits) and catalog (wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits.wcscat) found
'wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits.wcscat' -> 'wcsmag.cat'
Read 6437 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 143.5054 to 160.9805 deg, Dec +16.5181 to +27.2611 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 143.5054 to 160.9805 deg, Dec 16.5181 to 27.2611 deg
Loaded 4555 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): 3604 out of 3731 total matches.
Matched with Tycho-2 3731 out of 6437 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.758100
a=0.000000 b=1.000000 c=22.758100
From vast_summary.log: estimated ref. image limiting mag.: -7.28
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.48
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.48
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 6437 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 143.5054 to 160.9805 deg, Dec +16.5181 to +27.2611 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 143.5054 to 160.9805 deg, Dec 16.5181 to 27.2611 deg
Loaded 4555 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): 3604 out of 3731 total matches.
Matched with Tycho-2 3731 out of 6437 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits
Forced-photometry filter: calibrated wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits -> calib.txt_param_ref_wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits (aperture=6.6)
Read 6417 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 143.5056 to 160.9562 deg, Dec +16.5180 to +27.2611 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 143.5056 to 160.9562 deg, Dec 16.5180 to 27.2611 deg
Loaded 4551 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): 3597 out of 3736 total matches.
Matched with Tycho-2 3736 out of 6417 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits
Forced-photometry filter: calibrated wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits -> calib.txt_param_ref_wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits (aperture=6.6)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.5 pix Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits
2.5 pix Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits
2.3 pix fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits
2.3 pix fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits
Limiting magnitude estimates:
15.5 mag. Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits
15.5 mag. Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits
14.6 mag. fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits
14.6 mag. fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 11.5 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.NctIo1WiRn (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-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.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_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.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-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.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-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits' -> 'wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.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-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits
WCS_IMAGE_NAME=wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits
WCS-calibrated image found: wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits
Checking if the catalog wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits.wcscat corresponding to the image wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits alredy exist and is non-empty...
Catalog wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits.wcscat corresponding to the image wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits
WCS catalog name: wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.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=398, bad_region=0, passed=6437
Got 6437 stars (including 6029 good ones) from the SExtractor catalog wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits.wcscat
util/solve_plate_with_UCAC5 got 6437 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4509 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4495 matched stars entering correct_measured_positions(), 4495 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4495 matched stars entering correct_measured_positions(), 6437 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4509 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4495 matched stars entering correct_measured_positions(), 6437 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 4495 matched stars entering correct_measured_positions(), 6437 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 4495 stars left (next iteration limit 4944)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits N_match=4495 sigma_overall_arcsec=0.417 sigma_q1_arcsec=0.327 sigma_q2_arcsec=0.429 sigma_q3_arcsec=0.422 sigma_q4_arcsec=0.464 n_q1=1031 n_q2=1208 n_q3=977 n_q4=1279 worst_quadrant_to_overall_ratio=1.113
The image catalog is written to wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits -region wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.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.JFSHAdS7FC (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-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.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_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.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-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.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-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits' -> 'wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.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-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits
WCS_IMAGE_NAME=wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits
WCS-calibrated image found: wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits
Checking if the catalog wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits.wcscat corresponding to the image wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits alredy exist and is non-empty...
Catalog wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits.wcscat corresponding to the image wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits
WCS catalog name: wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.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=394, bad_region=0, passed=6417
Got 6417 stars (including 6016 good ones) from the SExtractor catalog wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits.wcscat
util/solve_plate_with_UCAC5 got 6417 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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4515 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4499 matched stars entering correct_measured_positions(), 4499 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4499 matched stars entering correct_measured_positions(), 6417 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4516 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4499 matched stars entering correct_measured_positions(), 6417 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 4499 matched stars entering correct_measured_positions(), 6417 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 4499 stars left (next iteration limit 4948)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits N_match=4499 sigma_overall_arcsec=0.434 sigma_q1_arcsec=0.359 sigma_q2_arcsec=0.454 sigma_q3_arcsec=0.416 sigma_q4_arcsec=0.482 n_q1=1024 n_q2=1216 n_q3=974 n_q4=1285 worst_quadrant_to_overall_ratio=1.110
The image catalog is written to wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits -region wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.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.5zKJfqSltk (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_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.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_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits
WCS_IMAGE_NAME=wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits
WCS-calibrated image found: wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits
Checking if the catalog wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits.wcscat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits.wcscat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits
WCS catalog name: wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.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=9, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=246, bad_region=0, passed=3602
Got 3602 stars (including 3351 good ones) from the SExtractor catalog wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits.wcscat
util/solve_plate_with_UCAC5 got 3602 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 945.2'
Seting catalog search parameters based on the expected field of view 945.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013128 (47.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010502 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.1 to 27.4)
Done reading UCAC5 zone files...
Matched 2997 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2983 matched stars entering correct_measured_positions(), 2983 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2983 matched stars entering correct_measured_positions(), 3602 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.1 to 27.4)
Done reading UCAC5 zone files...
Matched 2998 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2983 matched stars entering correct_measured_positions(), 3602 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 2983 matched stars entering correct_measured_positions(), 3602 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 2983 stars left (next iteration limit 3281)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=2983 robust_rms=11.109 arcsec worst_region_rms=20.744 arcsec outer_annulus_rms=20.744 arcsec
SIP_REFIT: SIP order 3 trial: matched=2983 robust_rms=0.662 arcsec worst_region_rms=0.872 arcsec outer_annulus_rms=0.829 arcsec
SIP_REFIT: SIP order 5 trial: matched=2983 robust_rms=0.459 arcsec worst_region_rms=0.613 arcsec outer_annulus_rms=0.526 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=2983 robust_rms_before=1.628 arcsec robust_rms_before_corrected=0.372 arcsec robust_rms_after=0.459 arcsec worst_region_rms_before=0.502 worst_region_rms_after=0.613 outer_annulus_rms_before=1.657 outer_annulus_rms_after=0.526
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.502 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits worst_region_rms_kept=0.502 arcsec robust_rms_kept=0.372 arcsec matched=2983
WCS_QUALITY_DIAG: file=fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits N_match=2983 sigma_overall_arcsec=0.392 sigma_q1_arcsec=0.360 sigma_q2_arcsec=0.513 sigma_q3_arcsec=0.342 sigma_q4_arcsec=0.398 n_q1=874 n_q2=590 n_q3=880 n_q4=639 worst_quadrant_to_overall_ratio=1.306
The image catalog is written to wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits -region wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.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.S3CGH0qGyp (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_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.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_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits
WCS_IMAGE_NAME=wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits
WCS-calibrated image found: wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits
Checking if the catalog wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits.wcscat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits.wcscat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits
WCS catalog name: wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.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=2, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=229, bad_region=0, passed=3626
Got 3626 stars (including 3393 good ones) from the SExtractor catalog wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits.wcscat
util/solve_plate_with_UCAC5 got 3626 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 945.0'
Seting catalog search parameters based on the expected field of view 945.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013125 (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 0.010500 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.1 to 27.4)
Done reading UCAC5 zone files...
Matched 3026 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3010 matched stars entering correct_measured_positions(), 3010 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3010 matched stars entering correct_measured_positions(), 3626 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.1 to 27.4)
Done reading UCAC5 zone files...
Matched 3025 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3010 matched stars entering correct_measured_positions(), 3626 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 3010 matched stars entering correct_measured_positions(), 3626 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 3010 stars left (next iteration limit 3311)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3010 robust_rms=11.503 arcsec worst_region_rms=21.062 arcsec outer_annulus_rms=21.062 arcsec
SIP_REFIT: SIP order 3 trial: matched=3010 robust_rms=0.712 arcsec worst_region_rms=0.878 arcsec outer_annulus_rms=0.878 arcsec
SIP_REFIT: SIP order 5 trial: matched=3010 robust_rms=0.461 arcsec worst_region_rms=0.591 arcsec outer_annulus_rms=0.510 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3010 robust_rms_before=1.539 arcsec robust_rms_before_corrected=0.372 arcsec robust_rms_after=0.461 arcsec worst_region_rms_before=0.503 worst_region_rms_after=0.591 outer_annulus_rms_before=1.482 outer_annulus_rms_after=0.510
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.503 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits worst_region_rms_kept=0.503 arcsec robust_rms_kept=0.372 arcsec matched=3010
WCS_QUALITY_DIAG: file=fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits N_match=3010 sigma_overall_arcsec=0.382 sigma_q1_arcsec=0.357 sigma_q2_arcsec=0.517 sigma_q3_arcsec=0.306 sigma_q4_arcsec=0.392 n_q1=867 n_q2=597 n_q3=893 n_q4=653 worst_quadrant_to_overall_ratio=1.355
The image catalog is written to wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits -region wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.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-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits to local_wcs_cache/
'wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits' -> 'local_wcs_cache/wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits'
Saving the final (post-refit) wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits to local_wcs_cache/
'wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits' -> 'local_wcs_cache/wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits'
Saving the final (post-refit) wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits to local_wcs_cache/
'wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits' -> 'local_wcs_cache/wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits'
Saving the final (post-refit) wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits to local_wcs_cache/
'wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits' -> 'local_wcs_cache/wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits sigma_overall=0.417 worst_q_ratio=1.113
ref2=Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits sigma_overall=0.434 worst_q_ratio=1.110
new1=fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits sigma_overall=0.392 worst_q_ratio=1.306
new2=fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits sigma_overall=0.382 worst_q_ratio=1.355
reference average sigma_overall=0.4255 worst_q_ratio=1.1115
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189_astrometric_residuals.png (4495 matched stars from wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.36 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190_astrometric_residuals.png (4499 matched stars from wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.38 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496_astrometric_residuals.png (2983 matched stars from wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.33 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497_astrometric_residuals.png (3010 matched stars from wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.32 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits'
Saving fully-calibrated image wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits'
Preparing the HTML report for the field Leo-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
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: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03676_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497
The candidate 03676_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497 did not pass the final checks
**** FOUND 10:00:01.94 +21:15:43.9 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Leo-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits
SExtractor catalog cache: saved Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits.cat to cache
SExtractor catalog cache: saved Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.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-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits
Creating symlink local_wcs_cache/wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.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-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits exists and is non-empty
wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits exists and is non-empty
wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits exists and is non-empty
wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits (1st reference image)
verification OK: wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits
Image size: 937.4'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: 10:09:13.907 +22:00:17.19 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-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits (1st new image)
verification OK: wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits
Image size: 945.2'x627.0' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 10:09:07.439 +21:56:58.14 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 10:09:13.907 +22:00:17.19
Second-epoch image center 10:09:07.439 +21:56:58.14
Angular distance between the image centers 0.0607 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits (2nd new image)
verification OK: wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits
Image size: 945.0'x627.0' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 10:09:08.624 +21:57:32.16 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 10:09:13.907 +22:00:17.19
Second-epoch image center 10:09:08.624 +21:57:32.16
Angular distance between the image centers 0.0502 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 10:09:07.439 +21:56:58.14
Second-epoch second image center 10:09:08.624 +21:57:32.16
Angular distance between the image centers 0.01050 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-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits &> /tmp/tmp.m11jFxzin4
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits &> /tmp/tmp.25vYSiBxXs
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits &> /tmp/tmp.4WIMWTePXH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits &> /tmp/tmp.BI3g8DmHJ6
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.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-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits and wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.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-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits and wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits.wcscat
Found non-empty wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits and wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits.wcscat
The reference image (wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits) and catalog (wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits.wcscat) found
'wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits.wcscat' -> 'wcsmag.cat'
Read 33023 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 143.5054 to 160.9804 deg, Dec +16.4875 to +27.2789 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 143.5054 to 160.9804 deg, Dec 16.4875 to 27.2789 deg
Loaded 4578 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): 3477 out of 3771 total matches.
Matched with Tycho-2 3771 out of 33023 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.649300
a=0.000000 b=1.000000 c=22.649300
From vast_summary.log: estimated ref. image limiting mag.: -7.03
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.62
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.62
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 33023 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 143.5054 to 160.9804 deg, Dec +16.4875 to +27.2789 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 143.5054 to 160.9804 deg, Dec 16.4875 to 27.2789 deg
Loaded 4578 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): 3477 out of 3771 total matches.
Matched with Tycho-2 3771 out of 33023 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits
Forced-photometry filter: calibrated wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits -> calib.txt_param_ref_wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits (aperture=5.2)
Read 33297 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 143.4723 to 160.9684 deg, Dec +16.4862 to +27.2734 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 143.4723 to 160.9684 deg, Dec 16.4862 to 27.2734 deg
Loaded 4585 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): 3482 out of 3773 total matches.
Matched with Tycho-2 3773 out of 33297 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits
Forced-photometry filter: calibrated wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits -> calib.txt_param_ref_wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits (aperture=5.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 29 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits
2.2 pix Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits
2.2 pix fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits
2.2 pix fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits
Limiting magnitude estimates:
15.6 mag. Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits
15.6 mag. Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits
14.8 mag. fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits
14.8 mag. fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 14.0 (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.m11jFxzin4 (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-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.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_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.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-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.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-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits' -> 'wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.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-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits
WCS_IMAGE_NAME=wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits
WCS-calibrated image found: wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits
Checking if the catalog wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits.wcscat corresponding to the image wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits alredy exist and is non-empty...
Catalog wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits.wcscat corresponding to the image wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits
WCS catalog name: wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.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=31, blended=1503, bad_region=0, passed=32992
Got 32992 stars (including 31441 good ones) from the SExtractor catalog wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits.wcscat
util/solve_plate_with_UCAC5 got 32992 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4506 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4495 matched stars entering correct_measured_positions(), 4495 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4495 matched stars entering correct_measured_positions(), 32992 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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4506 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4495 matched stars entering correct_measured_positions(), 32992 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 4495 matched stars entering correct_measured_positions(), 32992 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 4495 stars left (next iteration limit 4944)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.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-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits N_match=4495 sigma_overall_arcsec=0.412 sigma_q1_arcsec=0.321 sigma_q2_arcsec=0.418 sigma_q3_arcsec=0.409 sigma_q4_arcsec=0.468 n_q1=1013 n_q2=1215 n_q3=964 n_q4=1303 worst_quadrant_to_overall_ratio=1.136
The image catalog is written to wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits -region wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.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.25vYSiBxXs (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-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.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_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.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-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.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-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits' -> 'wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.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-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits
WCS_IMAGE_NAME=wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits
WCS-calibrated image found: wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits
Checking if the catalog wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits.wcscat corresponding to the image wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits alredy exist and is non-empty...
Catalog wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits.wcscat corresponding to the image wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits
WCS catalog name: wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.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=1479, bad_region=0, passed=33280
Got 33280 stars (including 31754 good ones) from the SExtractor catalog wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits.wcscat
util/solve_plate_with_UCAC5 got 33280 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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4509 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4498 matched stars entering correct_measured_positions(), 4498 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4498 matched stars entering correct_measured_positions(), 33280 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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4510 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4498 matched stars entering correct_measured_positions(), 33280 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4498 matched stars entering correct_measured_positions(), 33280 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 4498 stars left (next iteration limit 4947)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.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-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits N_match=4498 sigma_overall_arcsec=0.428 sigma_q1_arcsec=0.342 sigma_q2_arcsec=0.444 sigma_q3_arcsec=0.399 sigma_q4_arcsec=0.465 n_q1=1013 n_q2=1217 n_q3=964 n_q4=1304 worst_quadrant_to_overall_ratio=1.087
The image catalog is written to wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits -region wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.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.4WIMWTePXH (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_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.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_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits
WCS_IMAGE_NAME=wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits
WCS-calibrated image found: wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits
Checking if the catalog wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits.wcscat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits.wcscat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits
WCS catalog name: wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.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=753, bad_region=47, passed=22038
Got 22038 stars (including 21202 good ones) from the SExtractor catalog wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits.wcscat
util/solve_plate_with_UCAC5 got 22038 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 945.2'
Seting catalog search parameters based on the expected field of view 945.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013128 (47.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010502 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.1 to 27.4)
Done reading UCAC5 zone files...
Matched 4474 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4458 matched stars entering correct_measured_positions(), 4458 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4458 matched stars entering correct_measured_positions(), 22038 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.1 to 27.4)
Done reading UCAC5 zone files...
Matched 4475 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4458 matched stars entering correct_measured_positions(), 22038 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4458 matched stars entering correct_measured_positions(), 22038 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4458 stars left (next iteration limit 4903)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.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=4458 robust_rms=10.658 arcsec worst_region_rms=21.629 arcsec outer_annulus_rms=21.629 arcsec
SIP_REFIT: SIP order 3 trial: matched=4458 robust_rms=0.655 arcsec worst_region_rms=0.890 arcsec outer_annulus_rms=0.890 arcsec
SIP_REFIT: SIP order 5 trial: matched=4458 robust_rms=0.467 arcsec worst_region_rms=0.640 arcsec outer_annulus_rms=0.536 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4458 robust_rms_before=1.624 arcsec robust_rms_before_corrected=0.372 arcsec robust_rms_after=0.467 arcsec worst_region_rms_before=0.481 worst_region_rms_after=0.640 outer_annulus_rms_before=1.625 outer_annulus_rms_after=0.536
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.481 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits worst_region_rms_kept=0.481 arcsec robust_rms_kept=0.372 arcsec matched=4458
WCS_QUALITY_DIAG: file=fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits N_match=4458 sigma_overall_arcsec=0.382 sigma_q1_arcsec=0.349 sigma_q2_arcsec=0.505 sigma_q3_arcsec=0.348 sigma_q4_arcsec=0.390 n_q1=1368 n_q2=855 n_q3=1294 n_q4=941 worst_quadrant_to_overall_ratio=1.324
The image catalog is written to wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits -region wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.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.BI3g8DmHJ6 (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_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.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_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits
WCS_IMAGE_NAME=wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits
WCS-calibrated image found: wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits
Checking if the catalog wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits.wcscat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits.wcscat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits
WCS catalog name: wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=699, bad_region=46, passed=21906
Got 21906 stars (including 21124 good ones) from the SExtractor catalog wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits.wcscat
util/solve_plate_with_UCAC5 got 21906 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 945.0'
Seting catalog search parameters based on the expected field of view 945.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013125 (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 0.010500 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.1 to 27.4)
Done reading UCAC5 zone files...
Matched 4474 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4458 matched stars entering correct_measured_positions(), 4458 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4458 matched stars entering correct_measured_positions(), 21906 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.1 to 27.4)
Done reading UCAC5 zone files...
Matched 4473 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4457 matched stars entering correct_measured_positions(), 21906 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 4457 matched stars entering correct_measured_positions(), 21906 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4457 stars left (next iteration limit 4903)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.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=4457 robust_rms=10.890 arcsec worst_region_rms=22.137 arcsec outer_annulus_rms=22.137 arcsec
SIP_REFIT: SIP order 3 trial: matched=4457 robust_rms=0.699 arcsec worst_region_rms=0.925 arcsec outer_annulus_rms=0.925 arcsec
SIP_REFIT: SIP order 5 trial: matched=4457 robust_rms=0.473 arcsec worst_region_rms=0.605 arcsec outer_annulus_rms=0.518 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4457 robust_rms_before=1.533 arcsec robust_rms_before_corrected=0.367 arcsec robust_rms_after=0.473 arcsec worst_region_rms_before=0.493 worst_region_rms_after=0.605 outer_annulus_rms_before=1.427 outer_annulus_rms_after=0.518
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.493 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits worst_region_rms_kept=0.493 arcsec robust_rms_kept=0.367 arcsec matched=4457
WCS_QUALITY_DIAG: file=fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits N_match=4457 sigma_overall_arcsec=0.376 sigma_q1_arcsec=0.340 sigma_q2_arcsec=0.509 sigma_q3_arcsec=0.327 sigma_q4_arcsec=0.378 n_q1=1355 n_q2=859 n_q3=1285 n_q4=958 worst_quadrant_to_overall_ratio=1.353
The image catalog is written to wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits -region wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.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-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.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_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-07-34_20.00sec_-0.00C_LIGHTs_0496.fits
Saving fully-calibrated image wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.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_2026-10-08_CI_Leo-02-Q1b1x1_051017_TTUQ1b1x1_1118145_WQIgLXYJ/wcs_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497.fits
Preparing the HTML report for the field Leo-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits at 10:26:19.69 +20:20:32.0: 15.90 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits at 09:37:32.57 +21:23:11.2: 15.77 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits at 09:54:49.47 +19:24:25.6: 16.00 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits at 09:56:37.44 +18:09:06.6: 15.95 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits at 10:04:41.26 +26:29:52.5: 12.91 +/- 0.02 detection
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits at 09:39:05.75 +22:07:19.4: 12.99 +/- 0.02 detection
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits at 09:36:34.84 +20:20:00.4: 14.52 +/- 0.11 detection
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits at 09:42:41.53 +18:01:29.9: 15.77 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits at 09:54:49.47 +19:24:25.6: 16.02 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits at 10:04:41.26 +26:29:52.5: 12.94 +/- 0.02 detection
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits at 09:56:37.44 +18:09:06.6: 16.03 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits at 10:26:19.69 +20:20:32.0: 15.90 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits at 09:39:05.75 +22:07:19.4: 13.02 +/- 0.03 detection
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits at 09:37:32.57 +21:23:11.2: 15.84 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.01 +/- 0.02
Forced photometry reference-image weighted average: 12.92 +/- 0.02
Forced photometry filter REJECTED candidate at 09:39:05.75 +22:07:19.4: ref_mag=13.01 +/- 0.02 new_mean_mag=13.1224 delta=-0.12 (need > 0.90)
Forced photometry filter REJECTED candidate at 10:04:41.26 +26:29:52.5: ref_mag=12.92 +/- 0.02 new_mean_mag=12.9149 delta=0.01 (need > 0.90)
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits at 09:36:34.84 +20:20:00.4: 14.37 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.43 +/- 0.07
Forced photometry filter REJECTED candidate at 09:36:34.84 +20:20:00.4: ref_mag=14.43 +/- 0.07 new_mean_mag=14.5023 delta=-0.07 (need > 0.90)
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits at 09:53:45.36 +19:33:59.9: 15.95 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits at 09:42:15.69 +22:07:08.8: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits at 09:42:41.53 +18:01:29.9: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits at 09:53:45.36 +19:33:59.9: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits at 09:42:15.69 +22:07:08.8: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits at 10:26:11.57 +20:15:33.2: 13.45 +/- 0.04 detection
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits at 10:26:11.57 +20:15:33.2: 13.42 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.03
Forced photometry filter REJECTED candidate at 10:26:11.57 +20:15:33.2: ref_mag=13.44 +/- 0.03 new_mean_mag=13.3968 delta=0.04 (need > 0.90)
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits at 09:47:08.83 +19:16:21.6: 13.96 +/- 0.06 detection
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits at 09:47:08.83 +19:16:21.6: 13.82 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.88 +/- 0.04
Forced photometry filter REJECTED candidate at 09:47:08.83 +19:16:21.6: ref_mag=13.88 +/- 0.04 new_mean_mag=13.8007 delta=0.08 (need > 0.90)
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits at 09:58:58.79 +17:10:02.5: 15.90 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits at 09:40:19.69 +24:50:34.7: 14.78 +/- 0.13 detection
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits at 09:40:19.69 +24:50:34.7: 14.71 +/- 0.12 detection
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits at 09:58:58.79 +17:10:02.5: 15.91 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.74 +/- 0.09
Forced photometry filter REJECTED candidate at 09:40:19.69 +24:50:34.7: ref_mag=14.74 +/- 0.09 new_mean_mag=14.3579 delta=0.38 (need > 0.90)
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits at 09:36:47.32 +21:25:35.5: 14.91 +/- 0.16 detection
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits at 09:36:47.32 +21:25:35.5: 14.76 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.82 +/- 0.10
Forced photometry filter REJECTED candidate at 09:36:47.32 +21:25:35.5: ref_mag=14.82 +/- 0.10 new_mean_mag=14.6841 delta=0.14 (need > 0.90)
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits at 09:40:36.24 +21:35:38.5: 14.86 +/- 0.14 detection
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits at 09:40:36.24 +21:35:38.5: 14.70 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.77 +/- 0.09
Forced photometry filter REJECTED candidate at 09:40:36.24 +21:35:38.5: ref_mag=14.77 +/- 0.09 new_mean_mag=14.6205 delta=0.15 (need > 0.90)
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-29-48_20.00sec_-4.90C_LIGHT_0189.fits at 09:36:33.07 +24:53:20.9: 13.76 +/- 0.06 detection
Forced photometry on wcs_Leo-02-Q1b1x1_2026-04-09_00-30-39_20.00sec_-5.00C_LIGHT_0190.fits at 09:36:33.07 +24:53:20.9: 13.70 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.04
Forced photometry filter REJECTED candidate at 09:36:33.07 +24:53:20.9: ref_mag=13.73 +/- 0.04 new_mean_mag=13.6716 delta=0.06 (need > 0.90)
Adding exclusion_list_local.txt__out52900.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52908.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52936.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53147.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53202.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53213.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53351.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53775.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 18s
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: 6s
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Considering the candidate 52565_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497
The candidate 52565_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497 did not pass the final checks
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Considering the candidate 52572_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497
The candidate 52572_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497 did not pass the final checks
**** FOUND 09:44:10.21 +18:03:57.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52582_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497
The candidate 52582_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497 did not pass the final checks
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Considering the candidate 52583_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497
The candidate 52583_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497 did not pass the final checks
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Considering the candidate 52900_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497
Preparing report for the candidate 52900_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497
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Considering the candidate 52908_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497
Preparing report for the candidate 52908_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497
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Considering the candidate 52936_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497
Preparing report for the candidate 52936_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497
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Considering the candidate 52960_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497
The candidate 52960_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497 did not pass the final checks
**** FOUND 09:51:55.57 +24:21:46.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 53147_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497
Preparing report for the candidate 53147_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497
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Considering the candidate 53154_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497
The candidate 53154_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497 did not pass the final checks
**** FOUND 10:26:52.56 +19:22:41.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 53170_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497
The candidate 53170_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497 did not pass the final checks
**** FOUND 09:51:44.22 +20:10:33.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53179_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497
The candidate 53179_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497 did not pass the final checks
**** FOUND 09:36:02.37 +23:10:32.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53202_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497
Preparing report for the candidate 53202_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497
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Considering the candidate 53213_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497
Preparing report for the candidate 53213_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497
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Considering the candidate 53351_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497
Preparing report for the candidate 53351_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497
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Considering the candidate 53360_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497
The candidate 53360_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497 did not pass the final checks
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Considering the candidate 53378_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497
The candidate 53378_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497 did not pass the final checks
**** FOUND 09:59:30.77 +21:17:59.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53381_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497
The candidate 53381_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497 did not pass the final checks
**** FOUND 09:50:55.82 +20:47:14.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53479_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497
The candidate 53479_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497 did not pass the final checks
**** FOUND 09:42:13.75 +24:30:21.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53507_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497
The candidate 53507_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497 did not pass the final checks
**** FOUND 09:37:11.14 +21:24:16.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53587_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497
The candidate 53587_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497 did not pass the final checks
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Considering the candidate 53624_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497
The candidate 53624_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497 did not pass the final checks
**** FOUND 10:20:25.51 +25:40:58.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53760_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497
The candidate 53760_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497 did not pass the final checks
**** FOUND 09:36:28.67 +25:50:52.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53775_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497
Preparing report for the candidate 53775_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497
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Considering the candidate 53876_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497
The candidate 53876_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497 did not pass the final checks
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Considering the candidate 53947_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497
The candidate 53947_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497 did not pass the final checks
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Considering the candidate 53949_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497
The candidate 53949_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497 did not pass the final checks
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Considering the candidate 06094_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497
The candidate 06094_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497 did not pass the final checks
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Considering the candidate 18572_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497
The candidate 18572_fd_Leo-02-Q1b1x1_2026-10-08_05-08-42_20.00sec_0.00C_LIGHTs_0497 did not pass the final checks
