This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe
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 12.1931 2461172.6931 11.71 10:33:50.00 +26:16:50.8
206.54376 59.35288 galactic Leo Second-epoch detections are separated by 0.7" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.511 Davida -2 0 2 11.9 0 0
Forced photometry on wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits at 10:33:50.00 +26:16:50.8: 15.88 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits at 10:33:50.00 +26:16:50.8: 15.82 +/- 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 12.1931* 10 33 50.00 +26 16 50.8 11.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461172.6931,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260512.1931 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.1931 2461172.6931 12.44 10:33:33.75 +23:36:48.2
211.60136 58.75425 galactic Leo Second-epoch detections are separated by 0.4" and 6.7 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 12.6 -0 0
Forced photometry on wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits at 10:33:33.75 +23:36:48.2: 15.98 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits at 10:33:33.75 +23:36:48.2: 15.86 +/- 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 12.1931* 10 33 33.75 +23 36 48.2 12.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461172.6931,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260512.1931 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.1931 2461172.6931 13.88 10:31:37.88 +22:20:23.4
213.73266 57.99865 galactic Leo Second-epoch detections are separated by 1.1" and 6.7 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 14.1 0 0
Forced photometry on wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits at 10:31:37.88 +22:20:23.4: 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 10:31:37.88 +22:20:23.4: 16.03 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.1931* 10 31 37.88 +22 20 23.4 13.9 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461172.6931,13.88,0.05,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 20260512.1931 13.88CV 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 12.1931 2461172.6931 14.55 09:48:56.36 +23:22:45.7
207.66775 48.78641 galactic Leo Second-epoch detections are separated by 2.9" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.567 Eleutheria -3 3 4 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 09:48:56.36 +23:22:45.7: 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 09:48:56.36 +23:22:45.7: 16.11 +/- 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 12.1931* 09 48 56.36 +23 22 45.7 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
VARIABLE_NAME,2461172.6931,14.55,0.05,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 20260512.1931 14.55CV 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 12.1931 2461172.6931 14.67 10:18:51.84 +18:30:33.2
218.54216 53.94913 galactic Leo Second-epoch detections are separated by 2.6" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.361 Bononia -4 1 4 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 10:18:51.84 +18:30:33.2: 16.17 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits at 10:18:51.84 +18:30:33.2: 16.09 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.1931* 10 18 51.84 +18 30 33.2 14.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461172.6931,14.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260512.1931 14.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 12.1931 2461172.6931 14.88 10:09:43.57 +24:56:31.7
207.04988 53.76338 galactic Leo Second-epoch detections are separated by 3.2" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.856 Backlunda -2 0 2 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 10:09:43.57 +24:56:31.7: 16.25 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits at 10:09:43.57 +24:56:31.7: 16.16 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 12.1931* 10 09 43.57 +24 56 31.7 14.9 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461172.6931,14.88,0.05,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 20260512.1931 14.88CV 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: 2461172.69332612 12.05.2026 04:38:13.377 /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 7
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: 4 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): 7445
Objects passed selection criteria: 7441
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: 6957.5
Average stars matched: 6705 (96.3708 %)
Memory usage VmPeak: 112868 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun May 10 15:05:05 CDT 2026
VaST build number 1.0rc89-44-gd532a530
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon May 11 23:44:25 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: 2461172.69332612 12.05.2026 04:38:13.377 /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 23
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: 12 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): 36097
Objects passed selection criteria: 36006
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: 32743
Average stars matched: 31838.8 (97.2383 %)
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 Sun May 10 15:05:05 CDT 2026
VaST build number 1.0rc89-44-gd532a530
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon May 11 23:45:53 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_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.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_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.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: 2461172.69283073
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
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.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_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
WCS_IMAGE_NAME=wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
Field of view for the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits was not set. Trying to guess...
The guess is 605 arcmin.
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.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_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits
WCS_IMAGE_NAME=wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits
Field of view for the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits was not set. Trying to guess...
Entering WCS image calibration mode.
The guess is 605 arcmin.
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
No image with WCS calibration found for /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits .... Determining astrometry method...
Using the local copy of Astrometry.net software...
Choosing aperture...
Using the catalog image00003.cat SExtracted earlier from the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
No image with WCS calibration found for /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits .... Determining astrometry method...
Entering WCS image calibration mode.
Using the local copy of Astrometry.net software...
Choosing aperture...
Using the catalog image00004.cat SExtracted earlier from the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits
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
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/lib/make_outxyls_for_astrometric_calibration found 5925 high-SNR stars for plate solving
It's a known telescope with plate solutions that are supposed to be good.
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/workdir/vast_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/lib/make_outxyls_for_astrometric_calibration found 5922 high-SNR stars for plate solving
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_2026-01-18_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
Field of view for the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits was not set. Trying to guess...
'/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
Field of view for the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits was not set. Trying to guess...
The guess is 573 arcmin.
The guess is 573 arcmin.
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 was not found.
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
verification OK: 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_2026-02-21_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 was not found.
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
verification OK: wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
This service uses tools provided by Astrometry.net.
For more information visit http://astrometry.net/
This service uses tools provided by Astrometry.net.
For more information visit http://astrometry.net/
######### Trying to solve plate assuming 605' field of view #########
/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
Using the local copy of Astrometry.net code
######### Trying to solve plate assuming 605' field of view #########
/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits
Using the local copy of Astrometry.net code
IMAGE_SIZE= --width 9576 --height 6388 SCALE_LOW=544.5 SCALE_HIGH=3025.0
Using solve-field binary
/usr/local/astrometry/bin/solve-field
Generating wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat from image00001.cat
Generating wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits.cat from image00002.cat
Reading input file 1 of 1: "out2493315.xyls"...
IMAGE_SIZE= --width 9576 --height 6388 SCALE_LOW=544.5 SCALE_HIGH=3025.0
Using solve-field binary
/usr/local/astrometry/bin/solve-field
Reading input file 1 of 1: "out2493346.xyls"...
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 created.
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 created.
verification OK: wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
verification OK: wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
verification OK: wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
verification OK: wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.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
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
Image size: 941.6'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: 10:09:14.104 +22:00:00.95 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 6968 stars ###
'wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
### Converted positions of 6793 stars ###
'wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits.cat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/correct_sextractor_wcs_catalog_usingxy2sky2493753.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
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
'/data_ssd/NMW-TexasTech/workdir/vast_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/correct_sextractor_wcs_catalog_usingxy2sky2493752.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
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
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out2493315.axy"...
Field 1 did not solve (index index-4119.fits, field objects 1-10).
Field 1 did not solve (index index-4118.fits, field objects 1-10).
Field 1 did not solve (index index-4117.fits, field objects 1-10).
log-odds ratio 24.7003 (5.33604e+10), 3 match, 0 conflict, 5 distractors, 23 index.
RA,Dec = (152.336,22.0083), pixel scale 5.97116 arcsec/pix.
Hit/miss: Hit/miss: -+---+-+(best)--------------------------------------------------------------------------------------------
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Field 1: solved with index index-4116.fits.
Field 1 solved: writing to file ./out2493315.solved to indicate this.
Reading file "./out2493346.axy"...
Field 1 did not solve (index index-4119.fits, field objects 1-10).
Field: out2493315.xyls
Field center: (RA,Dec) = (152.338995, 22.012538) deg.
Field center: (RA H:M:S, Dec D:M:S) = (10:09:21.359, +22:00:45.137).
Field size: 15.7837 x 10.5686 degrees
Field rotation angle: up is -176.483 degrees E of N
Field parity: neg
Inserting WCS header... Field 1 did not solve (index index-4118.fits, field objects 1-10).
'/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits' -> 'fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits'
Field 1 did not solve (index index-4117.fits, field objects 1-10).
log-odds ratio 24.6892 (5.27704e+10), 3 match, 0 conflict, 5 distractors, 23 index.
RA,Dec = (152.346,22.0023), pixel scale 5.97107 arcsec/pix.
Hit/miss: Hit/miss: -+-+---+(best)--------------------------------------------------------------------------------------------
Field 1: solved with index index-4116.fits.
Field 1 solved: writing to file ./out2493346.solved to indicate this.
WCS keywords have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M May 11 23:44 fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
-rw-r--r-- 1 apache apache 12K May 11 23:44 out2493315.wcs
Inserting WCS header (1st iteration local)... Opening FITS image file fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits for reading... done!
Creating new image file (wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits)... done!
Field: out2493346.xyls
Field center: (RA,Dec) = (152.349670, 22.006760) deg.
Field center: (RA H:M:S, Dec D:M:S) = (10:09:23.921, +22:00:24.337).
Field size: 15.7837 x 10.5686 degrees
Field rotation angle: up is -176.483 degrees E of N
Field parity: neg
Inserting WCS header... '/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits' -> 'fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits'
WCS keywords have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M May 11 23:44 fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits
-rw-r--r-- 1 apache apache 12K May 11 23:44 out2493346.wcs
Inserting WCS header (1st iteration local)... Opening FITS image file fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits for reading... done!
Creating new image file (wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits)... done!
done!
done!
All done!
done
The WCS header appears to be added with no errors in /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits (fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits)
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration01' / astrometry.net run
Reading input file 1 of 1: "out2493315.xyls"...
All done!
done
The WCS header appears to be added with no errors in /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits (fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits)
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration01' / astrometry.net run
Reading input file 1 of 1: "out2493346.xyls"...
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
Reading file "./out2493315.axy"...
Only searching for solutions within 15.7117 degrees of RA,Dec (152.338,22.0118)
log-odds ratio 24.7003 (5.33604e+10), 3 match, 0 conflict, 5 distractors, 23 index.
RA,Dec = (152.336,22.0083), pixel scale 5.97116 arcsec/pix.
Hit/miss: Hit/miss: -+---+-+(best)--------------------------------------------------------------------------------------------
Field 1: solved with index index-4116.fits.
Field 1 solved: writing to file ./out2493315.solved to indicate this.
Field: out2493315.xyls
Field center: (RA,Dec) = (152.336566, 22.011115) deg.
Field center: (RA H:M:S, Dec D:M:S) = (10:09:20.776, +22:00:40.015).
Field size: 15.7673 x 10.573 degrees
Field rotation angle: up is -176.475 degrees E of N
Field parity: neg
Reading sort column "FLUX_APER"
Sorting sort column
mmapping input file
Copying table header.
Writing row 0
Done
Solving...
WCS keywords have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M May 11 23:44 fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
-rw-r--r-- 1 apache apache 12K May 11 23:44 out2493315.wcs
Inserting WCS header (2nd iteration local)... Opening FITS image file fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits for reading... done!
Creating new image file (wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits)... done!
Reading file "./out2493346.axy"...
Only searching for solutions within 15.7117 degrees of RA,Dec (152.349,22.006)
log-odds ratio 24.6892 (5.27704e+10), 3 match, 0 conflict, 5 distractors, 23 index.
RA,Dec = (152.346,22.0023), pixel scale 5.97107 arcsec/pix.
Hit/miss: Hit/miss: -+-+---+(best)--------------------------------------------------------------------------------------------
done!
Field 1: solved with index index-4116.fits.
Field 1 solved: writing to file ./out2493346.solved to indicate this.
Field: out2493346.xyls
Field center: (RA,Dec) = (152.347258, 22.005327) deg.
Field center: (RA H:M:S, Dec D:M:S) = (10:09:23.342, +22:00:19.176).
Field size: 15.7672 x 10.573 degrees
Field rotation angle: up is -176.474 degrees E of N
Field parity: neg
WCS keywords have been successfully stripped from all HDUs in the file.
-rw-r--r-- 1 apache apache 117M May 11 23:44 fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits
-rw-r--r-- 1 apache apache 12K May 11 23:44 out2493346.wcs
Inserting WCS header (2nd iteration local)... Opening FITS image file fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits for reading... done!
Creating new image file (wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits)... done!
done!
All done!
The WCS header appears to be added with no errors.
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration02' / astrometry.net run
The field of view is large: we'll try to run Astromety.net code on the image itself rather than a star list
Reading input file "wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits"...
Found an existing WCS header, will try to verify it.
Extracting sources...
All done!
The WCS header appears to be added with no errors.
Keyword does not exist
Keyword has been changed to:
VAST001 = 'wcs_image_calibration.sh' / VaST script name
Keyword does not exist
Keyword has been changed to:
VAST002 = 'local ' / ASTROMETRYNET_LOCAL_OR_REMOTE
Keyword does not exist
Keyword has been changed to:
VAST003 = 'local ' / PLATE_SOLVE_SERVER
Keyword does not exist
Keyword has been changed to:
VAST004 = 'iteration02' / astrometry.net run
The field of view is large: we'll try to run Astromety.net code on the image itself rather than a star list
Reading input file "wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits"...
Found an existing WCS header, will try to verify it.
Extracting sources...
simplexy: found 23820 sources.
simplexy: found 23750 sources.
Solving...
Reading file "./wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.axy"...
Verifying WCS using indices with quads of size [63.7114, 955.072] arcmin
Solving...
Verifying WCS with index 39 of 61 (/usr/local/astrometry/data/index-4117.fits)
Verifying WCS of field 1.
--> log-odds 8.18645
Verifying WCS with index 40 of 61 (/usr/local/astrometry/data/index-4116.fits)
Verifying WCS of field 1.
log-odds ratio 145.958 (2.44646e+63), 22 match, 0 conflict, 205 distractors, 23 index.
RA,Dec = (152.338,22.0119), pixel scale 5.98416 arcsec/pix.
Hit/miss: Hit/miss: -------+--------+----+---------------------------+-+-------+-----+---------+------+-------+---------
Reading file "./wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.axy"...
Verifying WCS using indices with quads of size [63.7116, 955.076] arcmin
Verifying WCS with index 39 of 61 (/usr/local/astrometry/data/index-4117.fits)
Verifying WCS of field 1.
--> log-odds 145.958
Verifying WCS with index 41 of 61 (/usr/local/astrometry/data/index-4115.fits)
Verifying WCS of field 1.
log-odds ratio 405.436 (1.19834e+176), 43 match, 0 conflict, 200 distractors, 44 index.
RA,Dec = (152.338,22.0119), pixel scale 5.98416 arcsec/pix.
Hit/miss: Hit/miss: -----+-+++------+--+-+----+-++------++-----------+-+-----+-+----++----+----+----+-+-------+---------
--> log-odds 17.9224
Verifying WCS with index 40 of 61 (/usr/local/astrometry/data/index-4116.fits)
Verifying WCS of field 1.
log-odds ratio 151.329 (5.26446e+65), 21 match, 0 conflict, 228 distractors, 23 index.
RA,Dec = (152.348,22.0061), pixel scale 5.98418 arcsec/pix.
Hit/miss: Hit/miss: -+--+---+----+-----+------+--------------+-----------------+---------------+------+-------+---------
--> log-odds 151.329
Verifying WCS with index 41 of 61 (/usr/local/astrometry/data/index-4115.fits)
Verifying WCS of field 1.
log-odds ratio 397.927 (6.56883e+172), 42 match, 0 conflict, 207 distractors, 44 index.
RA,Dec = (152.348,22.0061), pixel scale 5.98418 arcsec/pix.
Hit/miss: Hit/miss: -+--++--+----+-----+------+--+-----+-+---+-++-----+----++-++-----+---------+------+-------+-----+---
--> log-odds 405.436
Verifying WCS with index 42 of 61 (/usr/local/astrometry/data/index-4114.fits)
Verifying WCS of field 1.
log-odds ratio 810.563 (inf), 81 match, 0 conflict, 200 distractors, 83 index.
RA,Dec = (152.338,22.0119), pixel scale 5.98416 arcsec/pix.
Hit/miss: Hit/miss: +--+-+-+++-++---+-++-+--+-+-+++-----++--+-+-+---++-+----++++---+++++--+---+++---+-+++---+-++--+-+---
--> log-odds 397.927
Verifying WCS with index 42 of 61 (/usr/local/astrometry/data/index-4114.fits)
Verifying WCS of field 1.
log-odds ratio 808.797 (inf), 81 match, 0 conflict, 225 distractors, 83 index.
RA,Dec = (152.348,22.0061), pixel scale 5.98418 arcsec/pix.
Hit/miss: Hit/miss: ++--++--++++++--++-+--+--++--+--+--+-+--++-++---+-+-+--+++++--+--++-----+-++++--+-++------+-----+--+
--> log-odds 810.563
Verifying WCS with index 43 of 61 (/usr/local/astrometry/data/index-4113.fits)
Verifying WCS of field 1.
log-odds ratio 1832.02 (inf), 186 match, 0 conflict, 146 distractors, 191 index.
RA,Dec = (152.338,22.0119), pixel scale 5.98416 arcsec/pix.
Hit/miss: Hit/miss: ++-+-+++++++++++++++-++++++++++++++++++++++++++-+++++-++++++---+++++-++++++++++-++++++-++-+++++-++++
--> log-odds 808.797
Verifying WCS with index 43 of 61 (/usr/local/astrometry/data/index-4113.fits)
Verifying WCS of field 1.
log-odds ratio 1828.79 (inf), 186 match, 0 conflict, 138 distractors, 191 index.
RA,Dec = (152.348,22.0061), pixel scale 5.98418 arcsec/pix.
Hit/miss: Hit/miss: +++-+++-++++++++++++++++++++-+++++++-++++++++++-+-+++-++++++++++++++--+-+++++++-++++++-+-++++++-++++
--> log-odds 1832.02
Verifying WCS with index 44 of 61 (/usr/local/astrometry/data/index-4112.fits)
Verifying WCS of field 1.
log-odds ratio 3356.9 (inf), 363 match, 0 conflict, 486 distractors, 369 index.
RA,Dec = (152.338,22.0119), pixel scale 5.98416 arcsec/pix.
Hit/miss: Hit/miss: +++++++++++++++++++++++++++++++++++++++++++++++-++++++++++++++-+++++-+++++++++++++++++++++++++++++++
--> log-odds 1828.79
Verifying WCS with index 44 of 61 (/usr/local/astrometry/data/index-4112.fits)
Verifying WCS of field 1.
log-odds ratio 3356.92 (inf), 363 match, 0 conflict, 462 distractors, 369 index.
RA,Dec = (152.348,22.0061), pixel scale 5.98418 arcsec/pix.
Hit/miss: Hit/miss: +++++++++++++++++++++++++++++++++++++++++++++++-++++++++++++++++++++-++++++++++-++++++++++++++++++++
--> log-odds 3356.9
Verifying WCS with index 45 of 61 (/usr/local/astrometry/data/index-4111.fits)
Verifying WCS of field 1.
log-odds ratio 6130.81 (inf), 714 match, 0 conflict, 1152 distractors, 725 index.
RA,Dec = (152.338,22.0119), pixel scale 5.98416 arcsec/pix.
Hit/miss: Hit/miss: +++++++++++++++++++++++++++++++++++++++++++++++-++++++++++++++++++++++++++++++++++++++++++++++++++++
--> log-odds 3356.92
Verifying WCS with index 45 of 61 (/usr/local/astrometry/data/index-4111.fits)
Verifying WCS of field 1.
log-odds ratio 6127.42 (inf), 713 match, 0 conflict, 1106 distractors, 724 index.
RA,Dec = (152.348,22.0061), pixel scale 5.98418 arcsec/pix.
Hit/miss: Hit/miss: +++++++++++++++++++++++++++++++++++++++++++++++-++++++++++++++++++++++++++++++++++++++++++++++++++++
--> log-odds 6130.81
Verifying WCS with index 46 of 61 (/usr/local/astrometry/data/index-4110.fits)
Verifying WCS of field 1.
log-odds ratio 11349.6 (inf), 1440 match, 0 conflict, 2280 distractors, 1458 index.
RA,Dec = (152.338,22.0119), pixel scale 5.98416 arcsec/pix.
Hit/miss: Hit/miss: ++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++
--> log-odds 6127.42
Verifying WCS with index 46 of 61 (/usr/local/astrometry/data/index-4110.fits)
Verifying WCS of field 1.
log-odds ratio 11343 (inf), 1438 match, 0 conflict, 2283 distractors, 1456 index.
RA,Dec = (152.348,22.0061), pixel scale 5.98418 arcsec/pix.
Hit/miss: Hit/miss: ++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++
--> log-odds 11349.6
Got 7 solutions.
Field: wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
Field center: (RA,Dec) = (152.335607, 22.011494) deg.
Field center: (RA H:M:S, Dec D:M:S) = (10:09:20.546, +22:00:41.380).
Field size: 15.7676 x 10.57 degrees
Field rotation angle: up is -176.483 degrees E of N
Field parity: neg
Creating new FITS file "./wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.new"...
--> log-odds 11343
Got 7 solutions.
renamed 'wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.new' -> 'wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits'
Field: wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits
Field center: (RA,Dec) = (152.346315, 22.005697) deg.
Field center: (RA H:M:S, Dec D:M:S) = (10:09:23.116, +22:00:20.508).
Field size: 15.7676 x 10.57 degrees
Field rotation angle: up is -176.483 degrees E of N
Field parity: neg
Creating new FITS file "./wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.new"...
Checking if the catalog wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits.cat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits.cat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits was not found.
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
verification OK: wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
Generating wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits.cat from image00003.cat
renamed 'wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.new' -> 'wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits'
Catalog wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits.cat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits created.
verification OK: wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
Checking if the catalog wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits.cat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits.cat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits was not found.
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits
verification OK: wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits
Generating wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits.cat from image00004.cat
verification OK: wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
Catalog wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits.cat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits created.
verification OK: wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits
verification OK: wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.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: 10:09:20.318 +22:00:38.58 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 7110 stars ###
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: 10:09:22.888 +22:00:17.71 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
'wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits.cat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/correct_sextractor_wcs_catalog_usingxy2sky2512929.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
### Converted positions of 7110 stars ###
'wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits.cat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/correct_sextractor_wcs_catalog_usingxy2sky2512992.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits
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_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits exists and is non-empty
Saving wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits to local_wcs_cache/
'wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits' -> 'local_wcs_cache/wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits'
wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits exists and is non-empty
Saving wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits to local_wcs_cache/
'wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits' -> 'local_wcs_cache/wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.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_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits (1st new image)
verification OK: wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.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: 10:09:20.318 +22:00:38.58 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 10:09:20.318 +22:00:38.58
Angular distance between the image centers 0.0232 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits (2nd new image)
verification OK: wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.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: 10:09:22.888 +22:00:17.71 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 10:09:22.888 +22:00:17.71
Angular distance between the image centers 0.0313 deg.
###################################
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits sigma_overall=N/A worst_q_ratio=N/A
ref2=wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits sigma_overall=N/A worst_q_ratio=N/A
new1=wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits sigma_overall=N/A worst_q_ratio=N/A
new2=wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits sigma_overall=N/A worst_q_ratio=N/A
reference average sigma_overall=N/A worst_q_ratio=N/A
warn-on-ratio threshold: 2.0x reference
###################################
INFO: WCS quality sigma_overall_arcsec not available for comparison (1st new image new=N/A ref_avg=N/A)
INFO: WCS quality sigma_overall_arcsec not available for comparison (2nd new image new=N/A ref_avg=N/A)
INFO: WCS quality worst_quadrant_to_overall_ratio not available for comparison (1st new image new=N/A ref_avg=N/A)
INFO: WCS quality worst_quadrant_to_overall_ratio not available for comparison (2nd new image new=N/A ref_avg=N/A)
###################################
# 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 10:09:20.318 +22:00:38.58
Second-epoch second image center 10:09:22.888 +22:00:17.71
Angular distance between the image centers 0.01150 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.KejBMVsnZE
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.CretkdnK7J
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_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits &> /tmp/tmp.FZAO9X4mpG
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits &> /tmp/tmp.gGyMvCTm3k
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.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 7 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
3.8 pix fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
3.8 pix fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.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
15.0 mag. fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
15.0 mag. fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits
All-image limiting magnitude estimate: 15.0 (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.KejBMVsnZE (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_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/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.CretkdnK7J (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_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/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.FZAO9X4mpG (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_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.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_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
WCS_IMAGE_NAME=wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
WCS-calibrated image found: wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
Checking if the catalog wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits.cat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits.cat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.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_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
WCS catalog name: wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=296, passed=7110
Got 7110 stars (including 6812 good ones) from the SExtractor catalog wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits.cat
util/solve_plate_with_UCAC5 got 7110 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 887 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 887 matched stars entering correct_measured_positions(), 874 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 887 matched stars entering correct_measured_positions(), 7004 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 887 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 887 matched stars entering correct_measured_positions(), 7006 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 887 matched stars entering correct_measured_positions(), 7006 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 887 stars left (next iteration limit 975)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits N_match=887 sigma_overall_arcsec=0.326 sigma_q1_arcsec=0.309 sigma_q2_arcsec=0.474 sigma_q3_arcsec=0.274 sigma_q4_arcsec=0.289 n_q1=222 n_q2=219 n_q3=198 n_q4=248 worst_quadrant_to_overall_ratio=1.454
The image catalog is written to wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits -region wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.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.gGyMvCTm3k (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_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.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_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits
WCS_IMAGE_NAME=wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits
WCS-calibrated image found: wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits
Checking if the catalog wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits.cat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits.cat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.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_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits
WCS catalog name: wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=298, passed=7110
Got 7110 stars (including 6808 good ones) from the SExtractor catalog wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits.cat
util/solve_plate_with_UCAC5 got 7110 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 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(), 878 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 891 matched stars entering correct_measured_positions(), 7001 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.2 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(), 7002 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 891 matched stars entering correct_measured_positions(), 7002 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
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_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits N_match=891 sigma_overall_arcsec=0.316 sigma_q1_arcsec=0.307 sigma_q2_arcsec=0.471 sigma_q3_arcsec=0.244 sigma_q4_arcsec=0.271 n_q1=220 n_q2=222 n_q3=199 n_q4=250 worst_quadrant_to_overall_ratio=1.493
The image catalog is written to wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits -region wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits'
Saving fully-calibrated image wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.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 10:33:33.75 +23:36:48.2: 15.98 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits at 09:47:34.91 +26:12:55.9: 12.45 +/- 0.01 detection
Forced photometry on wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits at 10:00:36.82 +18:20:50.8: 12.80 +/- 0.02 detection
Forced photometry on wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits at 10:33:50.00 +26:16:50.8: 15.88 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits at 10:33:33.75 +23:36:48.2: 15.86 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits at 09:47:34.91 +26:12:55.9: 12.37 +/- 0.01 detection
Forced photometry on wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits at 10:33:50.00 +26:16:50.8: 15.82 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits at 10:00:36.82 +18:20:50.8: 12.81 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.41 +/- 0.01
Forced photometry filter REJECTED candidate at 09:47:34.91 +26:12:55.9: ref_mag=12.41 +/- 0.01 new_mean_mag=12.3033 delta=0.11 (need > 0.90)
Forced photometry reference-image weighted average: 12.80 +/- 0.01
Forced photometry filter REJECTED candidate at 10:00:36.82 +18:20:50.8: ref_mag=12.80 +/- 0.01 new_mean_mag=12.6116 delta=0.19 (need > 0.90)
Adding exclusion_list_local.txt__out20432.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20558.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
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: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20432_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093
Preparing report for the candidate 20432_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20482_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093
The candidate 20482_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093 did not pass the final checks
**** FOUND 10:07:32.27 +22:06:36.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20532_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093
The candidate 20532_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20558_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093
Preparing report for the candidate 20558_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20568_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093
The candidate 20568_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02295_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093
The candidate 02295_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093 did not pass the final checks
**** FOUND 09:43:25.73 +19:51:39.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06839_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093
The candidate 06839_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093 did not pass the final checks
**** FOUND 10:02:41.06 +26:41:35.2 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 8s
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 ####
10:33:50.00 +26:16:50.8
10:33:33.75 +23:36:48.2
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_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.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_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.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_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.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
Entering WCS image calibration mode.
Entering WCS image calibration mode.
Entering WCS image calibration mode.
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
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
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/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.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/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.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
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
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_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
WCS_IMAGE_NAME=wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
Field of view for the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits was not set. Trying to guess...
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 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_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits
WCS_IMAGE_NAME=wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits
Field of view for the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits was not set. Trying to guess...
The guess is 605 arcmin.
The guess is 605 arcmin.
WCS-calibrated image found: wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
Checking if the catalog wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits.cat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits.cat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits was not found.
WCS-calibrated image found: wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits
Checking if the catalog wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits.cat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits.cat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits was not found.
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits
It's a known telescope with plate solutions that are supposed to be good.
verification OK: wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
verification OK: wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits
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...
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_2026-01-18_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'
'/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_2026-01-18_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
Field of view for the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits was not set. Trying to guess...
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
Field of view for the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits was not set. Trying to guess...
The guess is 573 arcmin.
The guess is 573 arcmin.
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 was not found.
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 was not found.
verification OK: /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_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
verification OK: wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
verification OK: wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
Generating wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits.cat from image00003.cat
Generating wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits.cat from image00004.cat
Generating wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits.cat from image00002.cat
Generating wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat from image00001.cat
Catalog wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits.cat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits created.
verification OK: wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
Catalog wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits.cat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits created.
verification OK: wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits
verification OK: wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
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 created.
verification OK: wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
verification OK: wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits
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 created.
verification OK: wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
verification OK: wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
verification OK: wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.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: 10:09:20.318 +22:00:38.58 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
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: 10:09:22.888 +22:00:17.71 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
Image size: 941.6'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: 10:09:14.104 +22:00:00.95 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
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
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 28768 stars ###
'wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits.cat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/correct_sextractor_wcs_catalog_usingxy2sky2587391.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
### Converted positions of 28825 stars ###
'wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits.cat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/correct_sextractor_wcs_catalog_usingxy2sky2587400.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits
### Converted positions of 36566 stars ###
'wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits.cat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/correct_sextractor_wcs_catalog_usingxy2sky2587432.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
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
### Converted positions of 37822 stars ###
'wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/correct_sextractor_wcs_catalog_usingxy2sky2587453.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
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
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_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits exists and is non-empty
wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.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_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits (1st new image)
verification OK: wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
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: 10:09:20.318 +22:00:38.58 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 10:09:20.318 +22:00:38.58
Angular distance between the image centers 0.0232 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits (2nd new image)
verification OK: wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.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: 10:09:22.888 +22:00:17.71 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 10:09:22.888 +22:00:17.71
Angular distance between the image centers 0.0313 deg.
###################################
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits sigma_overall=N/A worst_q_ratio=N/A
ref2=wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits sigma_overall=N/A worst_q_ratio=N/A
new1=wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits sigma_overall=N/A worst_q_ratio=N/A
new2=wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits sigma_overall=N/A worst_q_ratio=N/A
reference average sigma_overall=N/A worst_q_ratio=N/A
warn-on-ratio threshold: 2.0x reference
###################################
INFO: WCS quality sigma_overall_arcsec not available for comparison (1st new image new=N/A ref_avg=N/A)
INFO: WCS quality sigma_overall_arcsec not available for comparison (2nd new image new=N/A ref_avg=N/A)
INFO: WCS quality worst_quadrant_to_overall_ratio not available for comparison (1st new image new=N/A ref_avg=N/A)
INFO: WCS quality worst_quadrant_to_overall_ratio not available for comparison (2nd new image new=N/A ref_avg=N/A)
###################################
# 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 10:09:20.318 +22:00:38.58
Second-epoch second image center 10:09:22.888 +22:00:17.71
Angular distance between the image centers 0.01150 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.07SvOFg6IL
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.RuO1aVAfrq
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_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits &> /tmp/tmp.1fVjDv6t5V
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits &> /tmp/tmp.2Fn72SY8vM
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.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 21 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
3.4 pix fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
3.4 pix fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.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
15.1 mag. fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
15.1 mag. fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits
All-image limiting magnitude estimate: 15.1 (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.07SvOFg6IL (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_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/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.RuO1aVAfrq (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_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/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.1fVjDv6t5V (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_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.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_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
WCS_IMAGE_NAME=wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
WCS-calibrated image found: wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
Checking if the catalog wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits.cat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits.cat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.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_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
WCS catalog name: wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=22, blended=1052, passed=28746
Got 28746 stars (including 27674 good ones) from the SExtractor catalog wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits.cat
util/solve_plate_with_UCAC5 got 28746 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 888 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 888 matched stars entering correct_measured_positions(), 879 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 888 matched stars entering correct_measured_positions(), 28482 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.1 to 27.5)
Done reading UCAC5 zone files...
Matched 888 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 888 matched stars entering correct_measured_positions(), 28481 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 888 matched stars entering correct_measured_positions(), 28481 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 888 stars left (next iteration limit 976)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits N_match=888 sigma_overall_arcsec=0.320 sigma_q1_arcsec=0.284 sigma_q2_arcsec=0.470 sigma_q3_arcsec=0.263 sigma_q4_arcsec=0.273 n_q1=217 n_q2=219 n_q3=205 n_q4=247 worst_quadrant_to_overall_ratio=1.467
The image catalog is written to wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits -region wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.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.2Fn72SY8vM (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_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.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_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits
WCS_IMAGE_NAME=wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits
WCS-calibrated image found: wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits
Checking if the catalog wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits.cat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits.cat corresponding to the image wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.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_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits
WCS catalog name: wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=1039, passed=28811
Got 28811 stars (including 27742 good ones) from the SExtractor catalog wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits.cat
util/solve_plate_with_UCAC5 got 28811 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(), 879 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 889 matched stars entering correct_measured_positions(), 28475 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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(), 28475 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 889 matched stars entering correct_measured_positions(), 28475 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
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_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits N_match=889 sigma_overall_arcsec=0.314 sigma_q1_arcsec=0.296 sigma_q2_arcsec=0.465 sigma_q3_arcsec=0.269 sigma_q4_arcsec=0.263 n_q1=219 n_q2=219 n_q3=202 n_q4=249 worst_quadrant_to_overall_ratio=1.481
The image catalog is written to wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits -region wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.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_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-37-30_20.00sec_-4.90C_LIGHTs_0092.fits
Saving fully-calibrated image wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.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_2026-05-11_CI_Leo-02-Q1b1x1_234213_TTUQ1b1x1_2482179_cRBzfwHe/wcs_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093.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 09:47:38.55 +18:01:58.2: 14.84 +/- 0.12 detection
Forced photometry on wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits at 09:36:35.27 +20:19:54.6: 14.27 +/- 0.07 detection
Forced photometry on wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits at 10:19:38.86 +22:31:49.9: 13.65 +/- 0.04 detection
Forced photometry on wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits at 09:41:48.54 +18:10:17.4: 14.58 +/- 0.10 detection
Forced photometry on wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits at 10:31:37.88 +22:20:23.4: 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 10:06:37.26 +17:54:43.6: 14.30 +/- 0.08 detection
Forced photometry on wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits at 09:48:56.36 +23:22:45.7: 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 10:35:01.37 +18:17:29.2: 15.47 +/- 0.23 detection
Forced photometry on wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits at 09:36:35.27 +20:19:54.6: 14.47 +/- 0.09 detection
Forced photometry on wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits at 10:19:38.86 +22:31:49.9: 13.70 +/- 0.05 detection
Forced photometry on wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits at 09:47:38.55 +18:01:58.2: 14.46 +/- 0.09 detection
Forced photometry on wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits at 09:41:48.54 +18:10:17.4: 14.71 +/- 0.11 detection
Forced photometry reference-image weighted average: 14.35 +/- 0.06
Forced photometry reference-image weighted average: 14.60 +/- 0.07
Forced photometry reference-image weighted average: 13.67 +/- 0.03
Forced photometry filter REJECTED candidate at 09:36:35.27 +20:19:54.6: ref_mag=14.35 +/- 0.06 new_mean_mag=14.1402 delta=0.21 (need > 0.90)
Forced photometry reference-image weighted average: 14.63 +/- 0.07
Forced photometry filter REJECTED candidate at 09:47:38.55 +18:01:58.2: ref_mag=14.60 +/- 0.07 new_mean_mag=14.6132 delta=-0.02 (need > 0.90)
Forced photometry filter REJECTED candidate at 10:19:38.86 +22:31:49.9: ref_mag=13.67 +/- 0.03 new_mean_mag=13.5878 delta=0.08 (need > 0.90)
Forced photometry filter REJECTED candidate at 09:41:48.54 +18:10:17.4: ref_mag=14.63 +/- 0.07 new_mean_mag=14.5423 delta=0.09 (need > 0.90)
Forced photometry on wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits at 10:18:51.84 +18:30:33.2: 16.17 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits at 10:09:43.57 +24:56:31.7: 16.25 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits at 10:31:37.88 +22:20:23.4: 16.03 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits at 10:06:37.26 +17:54:43.6: 14.18 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.23 +/- 0.05
Forced photometry on wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits at 09:48:56.36 +23:22:45.7: 16.11 +/- 99.00 upperlimit
Forced photometry filter REJECTED candidate at 10:06:37.26 +17:54:43.6: ref_mag=14.23 +/- 0.05 new_mean_mag=14.1575 delta=0.08 (need > 0.90)
Forced photometry on wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits at 10:35:01.37 +18:17:29.2: 15.07 +/- 0.17 detection
Forced photometry reference-image weighted average: 15.21 +/- 0.14
Forced photometry filter REJECTED candidate at 10:35:01.37 +18:17:29.2: ref_mag=15.21 +/- 0.14 new_mean_mag=14.9203 delta=0.29 (need > 0.90)
Forced photometry on wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits at 10:18:51.84 +18:30:33.2: 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 10:09:43.57 +24:56:31.7: 16.16 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q1b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits at 10:27:19.29 +25:36:45.3: 15.56 +/- 0.21 detection
Forced photometry on wcs_Leo-02-Q1b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits at 10:27:19.29 +25:36:45.3: 15.77 +/- 0.28 detection
Forced photometry reference-image weighted average: 15.63 +/- 0.17
Forced photometry filter REJECTED candidate at 10:27:19.29 +25:36:45.3: ref_mag=15.63 +/- 0.17 new_mean_mag=14.9951 delta=0.64 (need > 0.90)
Adding exclusion_list_local.txt__out52595.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53064.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53157.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53192.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 51844_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093
The candidate 51844_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093 did not pass the final checks
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Considering the candidate 51845_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093
The candidate 51845_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 51847_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093
The candidate 51847_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093 did not pass the final checks
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Considering the candidate 51850_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093
The candidate 51850_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093 did not pass the final checks
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Considering the candidate 52000_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093
The candidate 52000_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093 did not pass the final checks
**** FOUND 10:33:49.97 +26:16:50.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52124_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093
The candidate 52124_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093 did not pass the final checks
**** FOUND 10:33:33.74 +23:36:48.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52179_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093
The candidate 52179_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093 did not pass the final checks
**** FOUND 10:43:27.30 +24:48:03.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52249_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093
The candidate 52249_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093 did not pass the final checks
**** FOUND 10:26:52.51 +19:22:42.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 52264_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093
The candidate 52264_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093 did not pass the final checks
**** FOUND 10:23:52.05 +19:34:29.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52502_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093
The candidate 52502_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093 did not pass the final checks
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Considering the candidate 52595_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093
Preparing report for the candidate 52595_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093
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Considering the candidate 52665_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093
The candidate 52665_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093 did not pass the final checks
**** FOUND 09:38:36.02 +19:25:42.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52857_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093
The candidate 52857_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093 did not pass the final checks
**** FOUND 10:31:03.78 +22:13:40.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52886_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093
The candidate 52886_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093 did not pass the final checks
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Considering the candidate 53064_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093
Preparing report for the candidate 53064_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093
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Considering the candidate 53156_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093
The candidate 53156_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093 did not pass the final checks
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Considering the candidate 53157_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093
Preparing report for the candidate 53157_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093
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Considering the candidate 53192_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093
Preparing report for the candidate 53192_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093
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Considering the candidate 53198_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093
The candidate 53198_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093 did not pass the final checks
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Considering the candidate 12081_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093
The candidate 12081_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093 did not pass the final checks
**** FOUND 09:43:25.73 +19:51:39.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24797_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093
The candidate 24797_fd_Leo-02-Q1b1x1_2026-05-11_23-38-13_20.00sec_-5.00C_LIGHTs_0093 did not pass the final checks
