This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI
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 05 18.1709 2461178.6709 11.81 10:37:11.66 +25:37:47.2
208.07150 59.98489 galactic LMi Second-epoch detections are separated by 0.4" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.511 Davida -3 1 3 12.0 0 -0
Forced photometry on wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits at 10:37:11.66 +25:37:47.2: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits at 10:37:11.66 +25:37:47.2: 15.77 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461178.6709,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260518.1709 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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 05 18.1709* 10 29 51.60 +19 50 02.6 14.6 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
target,2461178.6709,14.56,0.05,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
target 20260518.1709 14.56CV 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 05 18.1709 2461178.6709 12.52 10:36:35.15 +22:41:00.8
213.68649 59.19316 galactic Leo Second-epoch detections are separated by 0.6" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.416 Vaticana -2 1 2 12.7 -0 0
Forced photometry on wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits at 10:36:35.15 +22:41:00.8: 16.06 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits at 10:36:35.15 +22:41:00.8: 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 05 18.1709* 10 36 35.15 +22 41 00.8 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,2461178.6709,12.52,0.05,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 20260518.1709 12.52CV 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 05 18.1709 2461178.6709 14.17 10:33:57.76 +21:35:15.9
215.38938 58.30462 galactic Leo Second-epoch detections are separated by 0.5" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.508 Princetonia -3 2 3 14.2 0 0
Forced photometry on wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits at 10:33:57.76 +21:35:15.9: 16.09 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits at 10:33:57.76 +21:35:15.9: 16.01 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 18.1709* 10 33 57.76 +21 35 15.9 14.2 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,2461178.6709,14.17,0.05,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 20260518.1709 14.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 18.1709 2461178.6709 14.40 09:53:31.36 +22:39:10.0
209.16914 49.60965 galactic Leo Second-epoch detections are separated by 2.8" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.567 Eleutheria -0 3 3 14.7 -0 0
Forced photometry on wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits at 09:53:31.36 +22:39:10.0: 16.23 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits at 09:53:31.36 +22:39:10.0: 16.13 +/- 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 05 18.1709* 09 53 31.36 +22 39 10.0 14.4 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,2461178.6709,14.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260518.1709 14.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 18.1709 2461178.6709 14.80 09:54:12.49 +17:32:50.6
216.60829 48.13494 galactic Leo Second-epoch detections are separated by 4.5" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.578 Happelia -3 -2 3 15.2 -0 0
Forced photometry on wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits at 09:54:12.49 +17:32:50.6: 16.15 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits at 09:54:12.49 +17:32:50.6: 16.01 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 18.1709* 09 54 12.49 +17 32 50.6 14.8 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,2461178.6709,14.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260518.1709 14.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 18.1709 2461178.6709 14.84 10:07:49.13 +18:13:29.2
217.43698 51.39965 galactic Leo Second-epoch detections are separated by 2.1" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.380 Fiducia -3 1 3 15.2 0 0
Forced photometry on wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits at 10:07:49.13 +18:13:29.2: 16.22 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits at 10:07:49.13 +18:13:29.2: 16.12 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 18.1709* 10 07 49.13 +18 13 29.2 14.8 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,2461178.6709,14.84,0.05,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 20260518.1709 14.84CV 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: 2461058.85568031 18.01.2026 08:32:00.779 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
First image: 2461058.85568031 18.01.2026 08:32:00.779 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
Last image: 2461178.67108829 18.05.2026 04:06:12.028 /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.46
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: 24
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
Total objects detected (at least 2 times): 7372
Objects passed selection criteria: 7366
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 6885
Average stars matched: 6655.25 (96.663 %)
Memory usage VmPeak: 112808 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed May 13 17:47:49 CDT 2026
VaST build number 1.0rc89-54-ga455e386
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-13)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun May 17 23:09:23 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: 2461058.85568031 18.01.2026 08:32:00.779 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
First image: 2461058.85568031 18.01.2026 08:32:00.779 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
Last image: 2461178.67108829 18.05.2026 04:06:12.028 /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 33
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.23
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 11 seconds
Number of parallel threads: 24
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
Total objects detected (at least 2 times): 36378
Objects passed selection criteria: 36292
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 33370.2
Average stars matched: 32467 (97.2932 %)
Memory usage VmPeak: 137516 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed May 13 17:47:49 CDT 2026
VaST build number 1.0rc89-54-ga455e386
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-13)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun May 17 23:10:50 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 --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits
SExtractor catalog cache: saved Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat to cache
SExtractor catalog cache: saved Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.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_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461178.67061800
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_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits exists and is non-empty
Saving wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits to local_wcs_cache/
'wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits' -> 'local_wcs_cache/wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits'
wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits exists and is non-empty
Saving wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits to local_wcs_cache/
'wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits' -> 'local_wcs_cache/wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits'
wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits exists and is non-empty
Saving wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits to local_wcs_cache/
'wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits' -> 'local_wcs_cache/wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits'
wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits exists and is non-empty
Saving wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits to local_wcs_cache/
'wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits' -> 'local_wcs_cache/wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits (1st reference image)
verification OK: wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
Image size: 941.7'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 10:09:14.835 +22:00:04.34 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits (1st new image)
verification OK: wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits
Image size: 941.0'x626.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.88"/pix along the Y axis
Image center: 10:09:26.937 +21:59:45.73 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 10:09:14.835 +22:00:04.34
Second-epoch image center 10:09:26.937 +21:59:45.73
Angular distance between the image centers 0.0470 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits (2nd new image)
verification OK: wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits
Image size: 941.0'x626.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.88"/pix along the Y axis
Image center: 10:09:27.116 +21:59:14.53 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 10:09:14.835 +22:00:04.34
Second-epoch image center 10:09:27.116 +21:59:14.53
Angular distance between the image centers 0.0494 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 10:09:26.937 +21:59:45.73
Second-epoch second image center 10:09:27.116 +21:59:14.53
Angular distance between the image centers 0.00869 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits &> /tmp/tmp.u0yWMwLljB
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits &> /tmp/tmp.CruPA9KJB9
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits &> /tmp/tmp.j71Xzkvbgp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits &> /tmp/tmp.Lh2VIUNCJu
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.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_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits and wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat
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_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits and wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat
Found non-empty wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits and wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat
The reference image (wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits) and catalog (wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat) found
'wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat' -> 'wcsmag.cat'
Read 6968 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 143.3687 to 160.8868 deg, Dec +16.3927 to +27.3357 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 143.3687 to 160.8868 deg, Dec 16.3927 to 27.3357 deg
Loaded 4674 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): 3606 out of 3801 total matches.
Matched with Tycho-2 3801 out of 6968 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.905550
a=0.000000 b=1.000000 c=22.905550
From vast_summary.log: estimated ref. image limiting mag.: -7.46
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.45
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.45
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 6968 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 143.3687 to 160.8868 deg, Dec +16.3927 to +27.3357 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 143.3687 to 160.8868 deg, Dec 16.3927 to 27.3357 deg
Loaded 4674 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): 3606 out of 3801 total matches.
Matched with Tycho-2 3801 out of 6968 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits:
Forced-photometry filter: calibrated wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits -> calib.txt_param_ref_wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits (aperture=6.1)
Read 6793 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 143.3688 to 160.8867 deg, Dec +16.3928 to +27.3358 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 143.3688 to 160.8867 deg, Dec 16.3928 to 27.3358 deg
Loaded 4674 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): 3603 out of 3798 total matches.
Matched with Tycho-2 3798 out of 6793 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits:
Forced-photometry filter: calibrated wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits -> calib.txt_param_ref_wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits (aperture=6.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
2.2 pix Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
3.2 pix fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits
3.1 pix fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits
2.0 pix wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
2.2 pix wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
Limiting magnitude estimates:
15.4 mag. Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
15.4 mag. Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
15.1 mag. fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits
15.1 mag. fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 12.4 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.u0yWMwLljB (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.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_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits' -> 'wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
WCS_IMAGE_NAME=wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
WCS-calibrated image found: wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
Checking if the catalog wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat corresponding to the image wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits alredy exist and is non-empty...
Catalog wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat corresponding to the image wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.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_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
WCS catalog name: wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=467, passed=6968
Got 6968 stars (including 6491 good ones) from the SExtractor catalog wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat
util/solve_plate_with_UCAC5 got 6968 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 910 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 909 matched stars entering correct_measured_positions(), 904 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 909 matched stars entering correct_measured_positions(), 6899 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 910 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 909 matched stars entering correct_measured_positions(), 6897 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 909 matched stars entering correct_measured_positions(), 6897 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 909 stars left (next iteration limit 999)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits N_match=909 sigma_overall_arcsec=0.316 sigma_q1_arcsec=0.369 sigma_q2_arcsec=0.340 sigma_q3_arcsec=0.313 sigma_q4_arcsec=0.259 n_q1=242 n_q2=222 n_q3=230 n_q4=215 worst_quadrant_to_overall_ratio=1.169
The image catalog is written to wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits -region wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.CruPA9KJB9 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.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_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits' -> 'wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
WCS_IMAGE_NAME=wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
WCS-calibrated image found: wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
Checking if the catalog wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits.cat corresponding to the image wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits alredy exist and is non-empty...
Catalog wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits.cat corresponding to the image wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.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_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
WCS catalog name: wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=460, passed=6793
Got 6793 stars (including 6327 good ones) from the SExtractor catalog wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits.cat
util/solve_plate_with_UCAC5 got 6793 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 909 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 908 matched stars entering correct_measured_positions(), 904 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 908 matched stars entering correct_measured_positions(), 6708 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
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 909 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 908 matched stars entering correct_measured_positions(), 6707 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 908 matched stars entering correct_measured_positions(), 6707 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 908 stars left (next iteration limit 998)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits N_match=908 sigma_overall_arcsec=0.371 sigma_q1_arcsec=0.439 sigma_q2_arcsec=0.340 sigma_q3_arcsec=0.340 sigma_q4_arcsec=0.369 n_q1=243 n_q2=222 n_q3=231 n_q4=212 worst_quadrant_to_overall_ratio=1.184
The image catalog is written to wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits -region wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.j71Xzkvbgp (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_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.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_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits
WCS_IMAGE_NAME=wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits
WCS-calibrated image found: wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits
Checking if the catalog wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits.cat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits.cat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.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_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits
WCS catalog name: wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=308, passed=6955
Got 6955 stars (including 6639 good ones) from the SExtractor catalog wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits.cat
util/solve_plate_with_UCAC5 got 6955 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 892 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 892 matched stars entering correct_measured_positions(), 881 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 892 matched stars entering correct_measured_positions(), 6832 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 892 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 892 matched stars entering correct_measured_positions(), 6832 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 892 matched stars entering correct_measured_positions(), 6832 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 892 stars left (next iteration limit 981)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits N_match=892 sigma_overall_arcsec=0.290 sigma_q1_arcsec=0.281 sigma_q2_arcsec=0.380 sigma_q3_arcsec=0.218 sigma_q4_arcsec=0.266 n_q1=217 n_q2=222 n_q3=202 n_q4=251 worst_quadrant_to_overall_ratio=1.309
The image catalog is written to wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits -region wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Lh2VIUNCJu (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_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.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_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits
WCS_IMAGE_NAME=wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits
WCS-calibrated image found: wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits
Checking if the catalog wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits.cat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits.cat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.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_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits
WCS catalog name: wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=333, passed=6977
Got 6977 stars (including 6639 good ones) from the SExtractor catalog wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits.cat
util/solve_plate_with_UCAC5 got 6977 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 892 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 892 matched stars entering correct_measured_positions(), 882 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 892 matched stars entering correct_measured_positions(), 6883 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 892 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 892 matched stars entering correct_measured_positions(), 6882 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 892 matched stars entering correct_measured_positions(), 6882 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 892 stars left (next iteration limit 981)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits N_match=892 sigma_overall_arcsec=0.278 sigma_q1_arcsec=0.270 sigma_q2_arcsec=0.374 sigma_q3_arcsec=0.238 sigma_q4_arcsec=0.250 n_q1=214 n_q2=227 n_q3=204 n_q4=247 worst_quadrant_to_overall_ratio=1.345
The image catalog is written to wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits -region wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits sigma_overall=0.316 worst_q_ratio=1.169
ref2=Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits sigma_overall=0.371 worst_q_ratio=1.184
new1=fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits sigma_overall=0.290 worst_q_ratio=1.309
new2=fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits sigma_overall=0.278 worst_q_ratio=1.345
reference average sigma_overall=0.3435 worst_q_ratio=1.1765
warn-on-ratio threshold: 2.0x reference
###################################
Distribution of catalog-matched stars across the image:
plot_astrometric_residuals_xy: wrote wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380_astrometric_residuals.png (909 matched stars from wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225_astrometric_residuals.png (908 matched stars from wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603_astrometric_residuals.png (892 matched stars from wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604_astrometric_residuals.png (892 matched stars from wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits.cat.astrometric_residuals, image 9576x6388)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits'
Saving fully-calibrated image wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits'
Preparing the HTML report for the field Leo-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits at 10:37:11.66 +25:37:47.2: 15.85 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits at 10:37:11.66 +25:37:47.2: 15.77 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out20444.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
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 20444_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604
Preparing report for the candidate 20444_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20470_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604
The candidate 20470_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604 did not pass the final checks
**** FOUND 10:16:48.85 +24:27:17.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20476_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604
The candidate 20476_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604 did not pass the final checks
**** FOUND 10:07:32.30 +22:06:36.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20536_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604
The candidate 20536_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604 did not pass the final checks
**** FOUND 09:47:34.88 +26:12:55.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02295_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604
The candidate 02295_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604 did not pass the final checks
**** FOUND 09:43:25.71 +19:51:39.7 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 6s
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 ####
10:37:11.66 +25:37:47.2
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits
SExtractor catalog cache: saved Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat to cache
SExtractor catalog cache: saved Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.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_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
Creating symlink local_wcs_cache/wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits exists and is non-empty
wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits exists and is non-empty
wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits exists and is non-empty
wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits (1st reference image)
verification OK: wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
Image size: 941.7'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 10:09:14.835 +22:00:04.34 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits (1st new image)
verification OK: wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits
Image size: 941.0'x626.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.88"/pix along the Y axis
Image center: 10:09:26.937 +21:59:45.73 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 10:09:14.835 +22:00:04.34
Second-epoch image center 10:09:26.937 +21:59:45.73
Angular distance between the image centers 0.0470 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits (2nd new image)
verification OK: wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits
Image size: 941.0'x626.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.88"/pix along the Y axis
Image center: 10:09:27.116 +21:59:14.53 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 10:09:14.835 +22:00:04.34
Second-epoch image center 10:09:27.116 +21:59:14.53
Angular distance between the image centers 0.0494 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 10:09:26.937 +21:59:45.73
Second-epoch second image center 10:09:27.116 +21:59:14.53
Angular distance between the image centers 0.00869 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits &> /tmp/tmp.Wv15OSwKHz
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits &> /tmp/tmp.Hed58AnGDE
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits &> /tmp/tmp.we7flmgOC5
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits &> /tmp/tmp.2z6lZCD0WD
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.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_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits and wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat
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_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits and wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat
Found non-empty wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits and wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat
The reference image (wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits) and catalog (wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat) found
'wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat' -> 'wcsmag.cat'
Read 37822 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 143.3687 to 160.9043 deg, Dec +16.3249 to +27.3468 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 143.3687 to 160.9043 deg, Dec 16.3249 to 27.3468 deg
Loaded 4718 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): 3458 out of 3819 total matches.
Matched with Tycho-2 3819 out of 37822 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.809000
a=0.000000 b=1.000000 c=22.809000
From vast_summary.log: estimated ref. image limiting mag.: -7.23
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.58
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.58
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 37822 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 143.3687 to 160.9043 deg, Dec +16.3249 to +27.3468 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 143.3687 to 160.9043 deg, Dec 16.3249 to 27.3468 deg
Loaded 4718 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): 3458 out of 3819 total matches.
Matched with Tycho-2 3819 out of 37822 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits:
Forced-photometry filter: calibrated wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits -> calib.txt_param_ref_wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits (aperture=4.9)
Read 36566 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 143.3688 to 160.9045 deg, Dec +16.3177 to +27.3431 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 143.3688 to 160.9045 deg, Dec 16.3177 to 27.3431 deg
Loaded 4721 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): 3449 out of 3818 total matches.
Matched with Tycho-2 3818 out of 36566 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits:
Forced-photometry filter: calibrated wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits -> calib.txt_param_ref_wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits (aperture=5.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 25 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
1.9 pix Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
2.1 pix Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
3.0 pix fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits
3.0 pix fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits
1.9 pix wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
2.1 pix wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
Limiting magnitude estimates:
15.6 mag. Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
15.5 mag. Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
15.2 mag. fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits
15.2 mag. fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits
All-image limiting magnitude estimate: 15.2 (SNR ) 14.5 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.Wv15OSwKHz (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.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_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits' -> 'wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
WCS_IMAGE_NAME=wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
WCS-calibrated image found: wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
Checking if the catalog wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat corresponding to the image wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits alredy exist and is non-empty...
Catalog wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat corresponding to the image wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.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_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
WCS catalog name: wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=1597, passed=37805
Got 37805 stars (including 36130 good ones) from the SExtractor catalog wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat
util/solve_plate_with_UCAC5 got 37805 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 903 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 902 matched stars entering correct_measured_positions(), 896 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 902 matched stars entering correct_measured_positions(), 37297 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 903 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 902 matched stars entering correct_measured_positions(), 37296 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 902 matched stars entering correct_measured_positions(), 37296 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 902 stars left (next iteration limit 992)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits N_match=902 sigma_overall_arcsec=0.316 sigma_q1_arcsec=0.342 sigma_q2_arcsec=0.337 sigma_q3_arcsec=0.330 sigma_q4_arcsec=0.250 n_q1=244 n_q2=223 n_q3=228 n_q4=207 worst_quadrant_to_overall_ratio=1.082
The image catalog is written to wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits -region wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Hed58AnGDE (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.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_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits' -> 'wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
WCS_IMAGE_NAME=wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
WCS-calibrated image found: wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
Checking if the catalog wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits.cat corresponding to the image wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits alredy exist and is non-empty...
Catalog wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits.cat corresponding to the image wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.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_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
WCS catalog name: wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=1590, passed=36546
Got 36546 stars (including 34883 good ones) from the SExtractor catalog wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits.cat
util/solve_plate_with_UCAC5 got 36546 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 903 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 902 matched stars entering correct_measured_positions(), 894 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 902 matched stars entering correct_measured_positions(), 36033 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
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 903 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 902 matched stars entering correct_measured_positions(), 36033 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 902 matched stars entering correct_measured_positions(), 36033 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 902 stars left (next iteration limit 992)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits N_match=902 sigma_overall_arcsec=0.356 sigma_q1_arcsec=0.402 sigma_q2_arcsec=0.330 sigma_q3_arcsec=0.344 sigma_q4_arcsec=0.337 n_q1=244 n_q2=221 n_q3=229 n_q4=208 worst_quadrant_to_overall_ratio=1.128
The image catalog is written to wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits -region wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.we7flmgOC5 (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_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.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_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits
WCS_IMAGE_NAME=wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits
WCS-calibrated image found: wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits
Checking if the catalog wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits.cat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits.cat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.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_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits
WCS catalog name: wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=1063, passed=30152
Got 30152 stars (including 29049 good ones) from the SExtractor catalog wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits.cat
util/solve_plate_with_UCAC5 got 30152 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.1 to 27.5)
Done reading UCAC5 zone files...
Matched 889 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 889 matched stars entering correct_measured_positions(), 878 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 889 matched stars entering correct_measured_positions(), 29726 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.1 to 27.5)
Done reading UCAC5 zone files...
Matched 889 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 889 matched stars entering correct_measured_positions(), 29726 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 889 matched stars entering correct_measured_positions(), 29727 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 889 stars left (next iteration limit 977)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits N_match=889 sigma_overall_arcsec=0.287 sigma_q1_arcsec=0.249 sigma_q2_arcsec=0.388 sigma_q3_arcsec=0.239 sigma_q4_arcsec=0.276 n_q1=216 n_q2=220 n_q3=205 n_q4=248 worst_quadrant_to_overall_ratio=1.352
The image catalog is written to wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits -region wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.2z6lZCD0WD (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_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.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_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits
WCS_IMAGE_NAME=wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits
WCS-calibrated image found: wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits
Checking if the catalog wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits.cat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits.cat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.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_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits
WCS catalog name: wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=1017, passed=29887
Got 29887 stars (including 28835 good ones) from the SExtractor catalog wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits.cat
util/solve_plate_with_UCAC5 got 29887 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.1 to 27.5)
Done reading UCAC5 zone files...
Matched 891 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 891 matched stars entering correct_measured_positions(), 884 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 891 matched stars entering correct_measured_positions(), 29577 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.1 to 27.5)
Done reading UCAC5 zone files...
Matched 891 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 891 matched stars entering correct_measured_positions(), 29578 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 891 matched stars entering correct_measured_positions(), 29578 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 891 stars left (next iteration limit 980)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits N_match=891 sigma_overall_arcsec=0.286 sigma_q1_arcsec=0.268 sigma_q2_arcsec=0.388 sigma_q3_arcsec=0.244 sigma_q4_arcsec=0.249 n_q1=213 n_q2=223 n_q3=208 n_q4=247 worst_quadrant_to_overall_ratio=1.358
The image catalog is written to wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits -region wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
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_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.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_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-05-31_20.00sec_-0.00C_LIGHTs_0603.fits
Saving fully-calibrated image wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.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_2026-05-17_CI_Leo-02-Q1b1x1_230710_TTUQ1b1x1_1144222_zYP20dUI/wcs_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604.fits
Preparing the HTML report for the field Leo-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits at 10:22:34.94 +24:00:58.7: 14.59 +/- 0.08 detection
Forced photometry on wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits at 10:36:35.15 +22:41:00.8: 16.06 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits at 10:06:37.40 +17:54:43.1: 14.23 +/- 0.07 detection
Forced photometry on wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits at 09:54:12.49 +17:32:50.6: 16.15 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits at 10:33:57.76 +21:35:15.9: 16.09 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits at 09:53:31.36 +22:39:10.0: 16.23 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits at 10:34:26.68 +20:59:46.9: 15.09 +/- 0.15 detection
Forced photometry on wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits at 10:36:35.15 +22:41:00.8: 16.02 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits at 09:43:47.65 +26:52:04.2: 14.02 +/- 0.06 detection
Forced photometry on wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits at 10:22:34.94 +24:00:58.7: 14.36 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.46 +/- 0.05
Forced photometry filter REJECTED candidate at 10:22:34.94 +24:00:58.7: ref_mag=14.46 +/- 0.05 new_mean_mag=14.5575 delta=-0.10 (need > 0.90)
Forced photometry on wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits at 10:06:37.40 +17:54:43.1: 14.13 +/- 0.07 detection
Forced photometry on wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits at 10:37:13.15 +25:31:05.6: 14.97 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.18 +/- 0.05
Forced photometry filter REJECTED candidate at 10:06:37.40 +17:54:43.1: ref_mag=14.18 +/- 0.05 new_mean_mag=14.1532 delta=0.03 (need > 0.90)
Forced photometry on wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits at 09:54:12.49 +17:32:50.6: 16.01 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits at 10:33:57.76 +21:35:15.9: 16.01 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits at 09:53:31.36 +22:39:10.0: 16.13 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits at 10:34:26.68 +20:59:46.9: 15.05 +/- 0.15 detection
Forced photometry reference-image weighted average: 15.07 +/- 0.11
Forced photometry filter REJECTED candidate at 10:34:26.68 +20:59:46.9: ref_mag=15.07 +/- 0.11 new_mean_mag=14.8106 delta=0.26 (need > 0.90)
Forced photometry on wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits at 09:43:47.65 +26:52:04.2: 14.03 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.02 +/- 0.04
Forced photometry filter REJECTED candidate at 09:43:47.65 +26:52:04.2: ref_mag=14.02 +/- 0.04 new_mean_mag=14.0602 delta=-0.04 (need > 0.90)
Forced photometry on wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits at 10:37:13.15 +25:31:05.6: 15.16 +/- 0.17 detection
Forced photometry reference-image weighted average: 15.04 +/- 0.11
Forced photometry filter REJECTED candidate at 10:37:13.15 +25:31:05.6: ref_mag=15.04 +/- 0.11 new_mean_mag=14.8109 delta=0.23 (need > 0.90)
Forced photometry on wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits at 10:38:08.32 +18:55:35.0: 14.87 +/- 0.14 detection
Forced photometry on wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits at 10:36:18.11 +22:22:25.9: 15.18 +/- 0.16 detection
Forced photometry on wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits at 10:21:32.54 +20:10:34.6: 15.27 +/- 0.15 detection
Forced photometry on wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits at 10:07:49.13 +18:13:29.2: 16.22 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits at 10:38:08.32 +18:55:35.0: 15.41 +/- 0.24 detection
Forced photometry reference-image weighted average: 15.01 +/- 0.12
Forced photometry filter REJECTED candidate at 10:38:08.32 +18:55:35.0: ref_mag=15.01 +/- 0.12 new_mean_mag=14.9083 delta=0.10 (need > 0.90)
Forced photometry on wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits at 10:36:18.11 +22:22:25.9: 15.10 +/- 0.16 detection
Forced photometry reference-image weighted average: 15.13 +/- 0.11
Forced photometry filter REJECTED candidate at 10:36:18.11 +22:22:25.9: ref_mag=15.13 +/- 0.11 new_mean_mag=14.9131 delta=0.22 (need > 0.90)
Forced photometry on wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits at 10:14:29.71 +22:11:58.5: 15.07 +/- 0.12 detection
Forced photometry on wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits at 10:21:32.54 +20:10:34.6: 15.59 +/- 0.22 detection
Forced photometry reference-image weighted average: 15.37 +/- 0.13
Forced photometry filter REJECTED candidate at 10:21:32.54 +20:10:34.6: ref_mag=15.37 +/- 0.13 new_mean_mag=14.7919 delta=0.58 (need > 0.90)
Forced photometry on wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits at 10:07:49.13 +18:13:29.2: 16.12 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits at 10:14:29.71 +22:11:58.5: 15.03 +/- 0.12 detection
Forced photometry reference-image weighted average: 15.05 +/- 0.09
Forced photometry filter REJECTED candidate at 10:14:29.71 +22:11:58.5: ref_mag=15.05 +/- 0.09 new_mean_mag=14.7768 delta=0.27 (need > 0.90)
Adding exclusion_list_local.txt__out52117.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52804.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52903.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53093.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53156.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 15s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 51843_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604
The candidate 51843_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 51846_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604
The candidate 51846_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604 did not pass the final checks
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Considering the candidate 51848_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604
Preparing report for the candidate 51848_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604
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Considering the candidate 52012_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604
The candidate 52012_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604 did not pass the final checks
**** FOUND 10:37:11.67 +25:37:47.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52117_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604
Preparing report for the candidate 52117_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604
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Considering the candidate 52162_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604
The candidate 52162_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604 did not pass the final checks
**** FOUND 10:43:27.27 +24:48:03.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52222_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604
The candidate 52222_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604 did not pass the final checks
**** FOUND 10:23:52.06 +19:34:29.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52229_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604
The candidate 52229_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604 did not pass the final checks
**** FOUND 10:26:52.50 +19:22:42.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 52614_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604
The candidate 52614_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604 did not pass the final checks
**** FOUND 09:46:06.08 +20:49:40.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52643_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604
The candidate 52643_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604 did not pass the final checks
**** FOUND 09:38:36.00 +19:25:43.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52720_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604
The candidate 52720_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604 did not pass the final checks
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Considering the candidate 52763_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604
The candidate 52763_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604 did not pass the final checks
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Considering the candidate 52804_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604
Preparing report for the candidate 52804_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604
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Considering the candidate 52886_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604
The candidate 52886_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604 did not pass the final checks
**** FOUND 10:31:03.65 +22:13:40.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52903_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604
Preparing report for the candidate 52903_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604
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Considering the candidate 53088_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604
The candidate 53088_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604 did not pass the final checks
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Considering the candidate 53093_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604
Preparing report for the candidate 53093_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604
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Considering the candidate 53102_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604
The candidate 53102_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604 did not pass the final checks
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Considering the candidate 53109_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604
The candidate 53109_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604 did not pass the final checks
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Considering the candidate 53116_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604
The candidate 53116_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604 did not pass the final checks
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Considering the candidate 53125_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604
The candidate 53125_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604 did not pass the final checks
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Considering the candidate 53156_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604
Preparing report for the candidate 53156_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604
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Considering the candidate 53217_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604
The candidate 53217_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604 did not pass the final checks
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Considering the candidate 12081_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604
The candidate 12081_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604 did not pass the final checks
**** FOUND 09:43:25.71 +19:51:39.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24797_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604
The candidate 24797_fd_Leo-02-Q1b1x1_2026-05-17_23-06-12_20.00sec_0.00C_LIGHTs_0604 did not pass the final checks
