This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 10 12.4797 2461325.9797 12.72 10:55:49.98 +02:33:26.9
249.57083 53.00751 galactic Leo Second-epoch detections are separated by 1.0" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.32 Pomona -1 -0 1 13.0 -0 0
Forced photometry on wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 10:55:49.98 +02:33:26.9: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 10:55:49.98 +02:33:26.9: 15.80 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 12.4797* 10 55 49.98 +02 33 26.9 12.7 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,2461325.9797,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261012.4797 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 12.4797 2461325.9797 13.07 10:43:54.36 +05:30:22.7
242.64189 52.74804 galactic Sex Second-epoch detections are separated by 2.3" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.43 Ariadne -0 1 1 13.2 0 -0
Forced photometry on wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 10:43:54.36 +05:30:22.7: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 10:43:54.36 +05:30:22.7: 15.75 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 12.4797* 10 43 54.36 +05 30 22.7 13.1 U Sex 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,2461325.9797,13.07,0.05,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 20261012.4797 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 12.4797 2461325.9797 13.71 10:43:52.89 +05:11:49.7
243.03040 52.54788 galactic Sex Second-epoch detections are separated by 2.7" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.194 Prokne -0 0 0 14.1 -0 -0
Forced photometry on wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 10:43:52.89 +05:11:49.7: 15.77 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 10:43:52.89 +05:11:49.7: 15.78 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 12.4797* 10 43 52.89 +05 11 49.7 13.7 U Sex 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,2461325.9797,13.71,0.05,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 20261012.4797 13.71CV 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 10 12.4797 2461325.9797 13.82 10:59:57.23 +04:45:59.7
248.05870 55.27757 galactic Leo Second-epoch detections are separated by 1.2" and 8.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.133 Cyrene -1 -1 1 14.1 0 -0
Forced photometry on wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 10:59:57.23 +04:45:59.7: 15.95 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 10:59:57.23 +04:45:59.7: 15.92 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 12.4797* 10 59 57.23 +04 45 59.7 13.8 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461325.9797,13.82,0.05,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 20261012.4797 13.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 12.4797 2461325.9797 13.70 11:05:07.70 +02:19:24.5
252.65054 54.46646 galactic Leo Second-epoch detections are separated by 2.0" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.218 Bianca 1 -0 1 14.1 0 -0
Forced photometry on wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 11:05:07.70 +02:19:24.5: 15.84 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 11:05:07.70 +02:19:24.5: 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 10 12.4797* 11 05 07.70 +02 19 24.5 13.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461325.9797,13.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261012.4797 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 10 12.4797 2461325.9797 13.96 10:59:51.57 +08:40:29.3
242.66527 57.81752 galactic Leo Second-epoch detections are separated by 3.8" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.261 Prymno 0 1 1 14.3 0 0
Forced photometry on wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 10:59:51.57 +08:40:29.3: 15.92 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 10:59:51.57 +08:40:29.3: 15.88 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 10 12.4797* 10 59 51.57 +08 40 29.3 14.0 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461325.9797,13.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261012.4797 13.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461149.73290969 19.04.2026 05:35:13.397 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
First image: 2461149.73290969 19.04.2026 05:35:13.397 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
Last image: 2461325.98006264 12.10.2026 11:31:07.412 /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 0
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.40
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 5353
Objects passed selection criteria: 5340
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 4078.25
Average stars matched: 3967.5 (97.2844 %)
Memory usage VmPeak: 231860 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Oct 9 16:07:04 CDT 2026
VaST build number 1.0rc89-234-g1a8c12b2
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-09)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Oct 12 06:34:55 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461149.73290969 19.04.2026 05:35:13.397 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
First image: 2461149.73290969 19.04.2026 05:35:13.397 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
Last image: 2461325.98006264 12.10.2026 11:31:07.412 /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 19
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.14
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 9 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 27046
Objects passed selection criteria: 26974
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 21891.5
Average stars matched: 21036.5 (96.0944 %)
Memory usage VmPeak: 251508 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Oct 9 16:07:04 CDT 2026
VaST build number 1.0rc89-234-g1a8c12b2
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-09)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Oct 12 06:35:36 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits
SExtractor catalog cache: saved Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.cat to cache
SExtractor catalog cache: saved Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461325.97932944
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits exists and is non-empty
wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits exists and is non-empty
wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits exists and is non-empty
wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits (1st reference image)
verification OK: wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
Image size: 937.5'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 11:08:41.747 +05:57:39.00 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits (1st new image)
verification OK: wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits
Image size: 945.0'x627.0' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:08:34.417 +06:00:13.09 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:08:41.747 +05:57:39.00
Second-epoch image center 11:08:34.417 +06:00:13.09
Angular distance between the image centers 0.0525 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits (2nd new image)
verification OK: wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits
Image size: 944.9'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:08:32.029 +06:00:49.42 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:08:41.747 +05:57:39.00
Second-epoch image center 11:08:32.029 +06:00:49.42
Angular distance between the image centers 0.0665 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 11:08:34.417 +06:00:13.09
Second-epoch second image center 11:08:32.029 +06:00:49.42
Angular distance between the image centers 0.01413 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits &> /tmp/tmp.CnItFGFAaG
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits &> /tmp/tmp.JSD0Mhwzju
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits &> /tmp/tmp.QlZxs4I1qW
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits &> /tmp/tmp.QIFgciexQN
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits and wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits and wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat
Found non-empty wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits and wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat
The reference image (wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits) and catalog (wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat) found
'wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat' -> 'wcsmag.cat'
Read 5626 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 159.1359 to 175.0748 deg, Dec +0.5733 to +11.2587 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 159.1359 to 175.0748 deg, Dec 0.5733 to 11.2587 deg
Loaded 3956 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3203 out of 3314 total matches.
Matched with Tycho-2 3314 out of 5626 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.762800
a=0.000000 b=1.000000 c=22.762800
From vast_summary.log: estimated ref. image limiting mag.: -7.40
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.36
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.36
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 5626 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 159.1359 to 175.0748 deg, Dec +0.5733 to +11.2587 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 159.1359 to 175.0748 deg, Dec 0.5733 to 11.2587 deg
Loaded 3956 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3203 out of 3314 total matches.
Matched with Tycho-2 3314 out of 5626 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
Forced-photometry filter: calibrated wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits -> calib.txt_param_ref_wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits (aperture=6.5)
Read 5579 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 159.1762 to 175.0853 deg, Dec +0.7334 to +11.2822 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 159.1762 to 175.0853 deg, Dec 0.7334 to 11.2822 deg
Loaded 3902 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3209 out of 3300 total matches.
Matched with Tycho-2 3300 out of 5579 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
Forced-photometry filter: calibrated wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits -> calib.txt_param_ref_wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits (aperture=6.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.4 pix Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
2.3 pix Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
2.5 pix fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits
2.5 pix fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits
Limiting magnitude estimates:
15.4 mag. Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
15.3 mag. Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
14.1 mag. fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits
14.1 mag. fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 11.2 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.CnItFGFAaG (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits' -> 'wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
WCS_IMAGE_NAME=wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
WCS-calibrated image found: wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
Checking if the catalog wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat corresponding to the image wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits alredy exist and is non-empty...
Catalog wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat corresponding to the image wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
WCS catalog name: wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=364, bad_region=0, passed=5626
Got 5626 stars (including 5255 good ones) from the SExtractor catalog wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat
util/solve_plate_with_UCAC5 got 5626 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 4819 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4806 matched stars entering correct_measured_positions(), 4806 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4806 matched stars entering correct_measured_positions(), 5626 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 4819 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4805 matched stars entering correct_measured_positions(), 5626 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4805 matched stars entering correct_measured_positions(), 5626 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 4805 stars left (next iteration limit 5286)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits N_match=4805 sigma_overall_arcsec=0.413 sigma_q1_arcsec=0.364 sigma_q2_arcsec=0.433 sigma_q3_arcsec=0.418 sigma_q4_arcsec=0.419 n_q1=1175 n_q2=1236 n_q3=1168 n_q4=1226 worst_quadrant_to_overall_ratio=1.048
The image catalog is written to wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits -region wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.JSD0Mhwzju (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits' -> 'wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
WCS_IMAGE_NAME=wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
WCS-calibrated image found: wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
Checking if the catalog wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.wcscat corresponding to the image wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits alredy exist and is non-empty...
Catalog wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.wcscat corresponding to the image wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
WCS catalog name: wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=3, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=329, bad_region=1, passed=5576
Got 5576 stars (including 5239 good ones) from the SExtractor catalog wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.wcscat
util/solve_plate_with_UCAC5 got 5576 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4825 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4813 matched stars entering correct_measured_positions(), 4813 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4813 matched stars entering correct_measured_positions(), 5576 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4825 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4813 matched stars entering correct_measured_positions(), 5576 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4813 matched stars entering correct_measured_positions(), 5576 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 4813 stars left (next iteration limit 5294)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits N_match=4813 sigma_overall_arcsec=0.418 sigma_q1_arcsec=0.325 sigma_q2_arcsec=0.472 sigma_q3_arcsec=0.370 sigma_q4_arcsec=0.476 n_q1=1150 n_q2=1248 n_q3=1173 n_q4=1242 worst_quadrant_to_overall_ratio=1.139
The image catalog is written to wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits -region wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.QlZxs4I1qW (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits
WCS_IMAGE_NAME=wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits
WCS-calibrated image found: wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits
Checking if the catalog wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits.wcscat corresponding to the image wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits.wcscat corresponding to the image wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits
WCS catalog name: wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=7, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=210, bad_region=0, passed=2643
Got 2643 stars (including 2432 good ones) from the SExtractor catalog wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits.wcscat
util/solve_plate_with_UCAC5 got 2643 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 945.0'
Seting catalog search parameters based on the expected field of view 945.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013125 (47.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010500 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 509 (Dec 0.3 to 11.5)
Done reading UCAC5 zone files...
Matched 2330 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2322 matched stars entering correct_measured_positions(), 2323 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2322 matched stars entering correct_measured_positions(), 2643 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 509 (Dec 0.3 to 11.5)
Done reading UCAC5 zone files...
Matched 2330 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2321 matched stars entering correct_measured_positions(), 2643 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 2321 matched stars entering correct_measured_positions(), 2643 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 2321 stars left (next iteration limit 2554)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=2321 robust_rms=10.309 arcsec worst_region_rms=21.400 arcsec outer_annulus_rms=21.400 arcsec
SIP_REFIT: SIP order 3 trial: matched=2321 robust_rms=0.591 arcsec worst_region_rms=0.809 arcsec outer_annulus_rms=0.809 arcsec
SIP_REFIT: SIP order 5 trial: matched=2321 robust_rms=0.340 arcsec worst_region_rms=0.465 arcsec outer_annulus_rms=0.381 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=2321 robust_rms_before=1.643 arcsec robust_rms_before_corrected=0.342 arcsec robust_rms_after=0.340 arcsec worst_region_rms_before=0.511 worst_region_rms_after=0.465 outer_annulus_rms_before=1.737 outer_annulus_rms_after=0.381
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.511 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits worst_region_rms_kept=0.511 arcsec robust_rms_kept=0.342 arcsec matched=2321
WCS_QUALITY_DIAG: file=fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits N_match=2321 sigma_overall_arcsec=0.350 sigma_q1_arcsec=0.367 sigma_q2_arcsec=0.463 sigma_q3_arcsec=0.283 sigma_q4_arcsec=0.330 n_q1=607 n_q2=475 n_q3=674 n_q4=565 worst_quadrant_to_overall_ratio=1.325
The image catalog is written to wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits -region wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.QIFgciexQN (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits
WCS_IMAGE_NAME=wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits
WCS-calibrated image found: wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits
Checking if the catalog wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits.wcscat corresponding to the image wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits.wcscat corresponding to the image wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits
WCS catalog name: wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=174, bad_region=0, passed=2615
Got 2615 stars (including 2437 good ones) from the SExtractor catalog wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits.wcscat
util/solve_plate_with_UCAC5 got 2615 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.9'
Seting catalog search parameters based on the expected field of view 944.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013124 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010499 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 509 (Dec 0.3 to 11.5)
Done reading UCAC5 zone files...
Matched 2337 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2327 matched stars entering correct_measured_positions(), 2329 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2327 matched stars entering correct_measured_positions(), 2615 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 509 (Dec 0.3 to 11.5)
Done reading UCAC5 zone files...
Matched 2336 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2326 matched stars entering correct_measured_positions(), 2615 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 2326 matched stars entering correct_measured_positions(), 2615 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 2326 stars left (next iteration limit 2559)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=2326 robust_rms=10.438 arcsec worst_region_rms=21.079 arcsec outer_annulus_rms=21.079 arcsec
SIP_REFIT: SIP order 3 trial: matched=2326 robust_rms=0.573 arcsec worst_region_rms=0.829 arcsec outer_annulus_rms=0.829 arcsec
SIP_REFIT: SIP order 5 trial: matched=2326 robust_rms=0.356 arcsec worst_region_rms=0.453 arcsec outer_annulus_rms=0.407 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=2326 robust_rms_before=1.668 arcsec robust_rms_before_corrected=0.336 arcsec robust_rms_after=0.356 arcsec worst_region_rms_before=0.460 worst_region_rms_after=0.453 outer_annulus_rms_before=1.709 outer_annulus_rms_after=0.407
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.460 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits worst_region_rms_kept=0.460 arcsec robust_rms_kept=0.336 arcsec matched=2326
WCS_QUALITY_DIAG: file=fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits N_match=2326 sigma_overall_arcsec=0.344 sigma_q1_arcsec=0.305 sigma_q2_arcsec=0.496 sigma_q3_arcsec=0.284 sigma_q4_arcsec=0.345 n_q1=624 n_q2=474 n_q3=670 n_q4=558 worst_quadrant_to_overall_ratio=1.440
The image catalog is written to wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits -region wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits to local_wcs_cache/
'wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits' -> 'local_wcs_cache/wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits'
Saving the final (post-refit) wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits to local_wcs_cache/
'wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits' -> 'local_wcs_cache/wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits'
Saving the final (post-refit) wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits to local_wcs_cache/
'wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits' -> 'local_wcs_cache/wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits'
Saving the final (post-refit) wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits to local_wcs_cache/
'wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits' -> 'local_wcs_cache/wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits sigma_overall=0.413 worst_q_ratio=1.048
ref2=Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits sigma_overall=0.418 worst_q_ratio=1.139
new1=fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits sigma_overall=0.350 worst_q_ratio=1.325
new2=fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits sigma_overall=0.344 worst_q_ratio=1.440
reference average sigma_overall=0.4155 worst_q_ratio=1.0935
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503_astrometric_residuals.png (4805 matched stars from wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148_astrometric_residuals.png (4813 matched stars from wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546_astrometric_residuals.png (2321 matched stars from wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.30 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547_astrometric_residuals.png (2326 matched stars from wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.30 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits'
Saving fully-calibrated image wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits'
Preparing the HTML report for the field Leo-07-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Leo-07-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits
SExtractor catalog cache: saved Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.cat to cache
SExtractor catalog cache: saved Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
Creating symlink local_wcs_cache/wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits exists and is non-empty
wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits exists and is non-empty
wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits exists and is non-empty
wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits (1st reference image)
verification OK: wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
Image size: 937.5'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 11:08:41.747 +05:57:39.00 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits (1st new image)
verification OK: wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits
Image size: 945.0'x627.0' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:08:34.417 +06:00:13.09 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:08:41.747 +05:57:39.00
Second-epoch image center 11:08:34.417 +06:00:13.09
Angular distance between the image centers 0.0525 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits (2nd new image)
verification OK: wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits
Image size: 944.9'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:08:32.029 +06:00:49.42 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:08:41.747 +05:57:39.00
Second-epoch image center 11:08:32.029 +06:00:49.42
Angular distance between the image centers 0.0665 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 11:08:34.417 +06:00:13.09
Second-epoch second image center 11:08:32.029 +06:00:49.42
Angular distance between the image centers 0.01413 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits &> /tmp/tmp.FTGsDo1tSo
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits &> /tmp/tmp.Icku6trb31
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits &> /tmp/tmp.XM30s6YDHQ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits &> /tmp/tmp.OPNQ1jnYqF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits and wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits and wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat
Found non-empty wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits and wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat
The reference image (wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits) and catalog (wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat) found
'wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat' -> 'wcsmag.cat'
Read 29706 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 159.1348 to 175.0760 deg, Dec +0.5733 to +11.2606 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 159.1348 to 175.0760 deg, Dec 0.5733 to 11.2606 deg
Loaded 3958 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3142 out of 3395 total matches.
Matched with Tycho-2 3395 out of 29706 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.644650
a=0.000000 b=1.000000 c=22.644650
From vast_summary.log: estimated ref. image limiting mag.: -7.14
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.50
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.50
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 29706 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 159.1348 to 175.0760 deg, Dec +0.5733 to +11.2606 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 159.1348 to 175.0760 deg, Dec 0.5733 to 11.2606 deg
Loaded 3958 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3142 out of 3395 total matches.
Matched with Tycho-2 3395 out of 29706 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
Forced-photometry filter: calibrated wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits -> calib.txt_param_ref_wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits (aperture=5.1)
Read 29098 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 159.1762 to 175.0872 deg, Dec +0.7305 to +11.2848 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 159.1762 to 175.0872 deg, Dec 0.7305 to 11.2848 deg
Loaded 3903 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3155 out of 3382 total matches.
Matched with Tycho-2 3382 out of 29098 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
Forced-photometry filter: calibrated wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits -> calib.txt_param_ref_wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits (aperture=5.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 16 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
2.2 pix Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
2.5 pix fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits
2.5 pix fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits
Limiting magnitude estimates:
15.5 mag. Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
15.5 mag. Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
14.3 mag. fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits
14.3 mag. fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 13.5 (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 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.FTGsDo1tSo (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits' -> 'wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
WCS_IMAGE_NAME=wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
WCS-calibrated image found: wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
Checking if the catalog wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat corresponding to the image wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits alredy exist and is non-empty...
Catalog wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat corresponding to the image wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits
WCS catalog name: wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=1187, bad_region=0, passed=29686
Got 29686 stars (including 28458 good ones) from the SExtractor catalog wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat
util/solve_plate_with_UCAC5 got 29686 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 4811 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4798 matched stars entering correct_measured_positions(), 4798 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4798 matched stars entering correct_measured_positions(), 29686 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 4811 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4798 matched stars entering correct_measured_positions(), 29686 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4798 matched stars entering correct_measured_positions(), 29686 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4798 stars left (next iteration limit 5277)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits N_match=4798 sigma_overall_arcsec=0.404 sigma_q1_arcsec=0.354 sigma_q2_arcsec=0.418 sigma_q3_arcsec=0.403 sigma_q4_arcsec=0.410 n_q1=1127 n_q2=1275 n_q3=1148 n_q4=1248 worst_quadrant_to_overall_ratio=1.035
The image catalog is written to wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits -region wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.Icku6trb31 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits' -> 'wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
WCS_IMAGE_NAME=wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
WCS-calibrated image found: wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
Checking if the catalog wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.wcscat corresponding to the image wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits alredy exist and is non-empty...
Catalog wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.wcscat corresponding to the image wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits
WCS catalog name: wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=1226, bad_region=1, passed=29081
Got 29081 stars (including 27822 good ones) from the SExtractor catalog wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.wcscat
util/solve_plate_with_UCAC5 got 29081 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4822 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4809 matched stars entering correct_measured_positions(), 4809 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4809 matched stars entering correct_measured_positions(), 29081 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4822 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4809 matched stars entering correct_measured_positions(), 29081 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4809 matched stars entering correct_measured_positions(), 29081 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4809 stars left (next iteration limit 5289)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits N_match=4809 sigma_overall_arcsec=0.397 sigma_q1_arcsec=0.322 sigma_q2_arcsec=0.444 sigma_q3_arcsec=0.362 sigma_q4_arcsec=0.449 n_q1=1165 n_q2=1236 n_q3=1196 n_q4=1212 worst_quadrant_to_overall_ratio=1.130
The image catalog is written to wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits -region wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.XM30s6YDHQ (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits
WCS_IMAGE_NAME=wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits
WCS-calibrated image found: wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits
Checking if the catalog wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits.wcscat corresponding to the image wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits.wcscat corresponding to the image wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits
WCS catalog name: wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=1, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=394, bad_region=22, passed=14701
Got 14701 stars (including 14267 good ones) from the SExtractor catalog wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits.wcscat
util/solve_plate_with_UCAC5 got 14701 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 945.0'
Seting catalog search parameters based on the expected field of view 945.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013125 (47.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010500 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 4795 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4783 matched stars entering correct_measured_positions(), 4783 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4783 matched stars entering correct_measured_positions(), 14701 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 4796 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4786 matched stars entering correct_measured_positions(), 14701 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 4786 matched stars entering correct_measured_positions(), 14701 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 4786 stars left (next iteration limit 5261)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4786 robust_rms=10.091 arcsec worst_region_rms=21.608 arcsec outer_annulus_rms=21.608 arcsec
SIP_REFIT: SIP order 3 trial: matched=4786 robust_rms=0.644 arcsec worst_region_rms=0.880 arcsec outer_annulus_rms=0.880 arcsec
SIP_REFIT: SIP order 5 trial: matched=4786 robust_rms=0.415 arcsec worst_region_rms=0.575 arcsec outer_annulus_rms=0.469 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4786 robust_rms_before=1.674 arcsec robust_rms_before_corrected=0.388 arcsec robust_rms_after=0.415 arcsec worst_region_rms_before=0.510 worst_region_rms_after=0.575 outer_annulus_rms_before=1.840 outer_annulus_rms_after=0.469
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.510 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits worst_region_rms_kept=0.510 arcsec robust_rms_kept=0.388 arcsec matched=4786
WCS_QUALITY_DIAG: file=fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits N_match=4786 sigma_overall_arcsec=0.382 sigma_q1_arcsec=0.373 sigma_q2_arcsec=0.501 sigma_q3_arcsec=0.330 sigma_q4_arcsec=0.363 n_q1=1326 n_q2=918 n_q3=1454 n_q4=1088 worst_quadrant_to_overall_ratio=1.312
The image catalog is written to wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits -region wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.OPNQ1jnYqF (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits
WCS_IMAGE_NAME=wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits
WCS-calibrated image found: wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits
Checking if the catalog wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits.wcscat corresponding to the image wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits.wcscat corresponding to the image wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits
WCS catalog name: wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=1, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=625, bad_region=22, passed=14936
Got 14936 stars (including 14271 good ones) from the SExtractor catalog wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits.wcscat
util/solve_plate_with_UCAC5 got 14936 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.9'
Seting catalog search parameters based on the expected field of view 944.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013124 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010499 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 4788 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4774 matched stars entering correct_measured_positions(), 4775 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4774 matched stars entering correct_measured_positions(), 14936 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 451 to 510 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 4787 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4774 matched stars entering correct_measured_positions(), 14936 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4774 matched stars entering correct_measured_positions(), 14936 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4774 stars left (next iteration limit 5251)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4774 robust_rms=10.369 arcsec worst_region_rms=21.361 arcsec outer_annulus_rms=21.361 arcsec
SIP_REFIT: SIP order 3 trial: matched=4774 robust_rms=0.642 arcsec worst_region_rms=0.893 arcsec outer_annulus_rms=0.893 arcsec
SIP_REFIT: SIP order 5 trial: matched=4774 robust_rms=0.430 arcsec worst_region_rms=0.556 arcsec outer_annulus_rms=0.512 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4774 robust_rms_before=1.697 arcsec robust_rms_before_corrected=0.391 arcsec robust_rms_after=0.430 arcsec worst_region_rms_before=0.523 worst_region_rms_after=0.556 outer_annulus_rms_before=1.749 outer_annulus_rms_after=0.512
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.523 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits worst_region_rms_kept=0.523 arcsec robust_rms_kept=0.391 arcsec matched=4774
WCS_QUALITY_DIAG: file=fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits N_match=4774 sigma_overall_arcsec=0.377 sigma_q1_arcsec=0.363 sigma_q2_arcsec=0.499 sigma_q3_arcsec=0.310 sigma_q4_arcsec=0.376 n_q1=1318 n_q2=929 n_q3=1443 n_q4=1084 worst_quadrant_to_overall_ratio=1.322
The image catalog is written to wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits -region wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-30-04_20.00sec_-0.00C_LIGHTs_0546.fits
Saving fully-calibrated image wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-10-12_CI_Leo-07-Q1b1x1_063158_TTUQ1b1x1_1637470_UrArOGPn/wcs_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547.fits
Preparing the HTML report for the field Leo-07-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 10:38:16.68 +08:24:36.5: 13.75 +/- 0.06 detection
Forced photometry on wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 10:55:49.98 +02:33:26.9: 15.81 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 10:39:45.07 +06:01:51.5: 13.42 +/- 0.04 detection
Forced photometry on wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 10:51:31.55 +05:28:00.8: 13.43 +/- 0.04 detection
Forced photometry on wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 11:33:01.22 +09:37:21.4: 11.20 +/- 0.01 detection
Forced photometry on wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 10:43:54.36 +05:30:22.7: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 10:59:57.23 +04:45:59.7: 15.95 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 11:04:58.18 +07:22:13.4: 13.44 +/- 0.04 detection
Forced photometry on wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 10:43:52.89 +05:11:49.7: 15.77 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 10:39:45.07 +06:01:51.5: 13.45 +/- 0.04 detection
Forced photometry on wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 10:51:31.55 +05:28:00.8: 13.60 +/- 0.05 detection
Forced photometry on wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 10:38:16.68 +08:24:36.5: 13.72 +/- 0.06 detection
Forced photometry on wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 11:33:01.22 +09:37:21.4: 11.27 +/- 0.01 detection
Forced photometry reference-image weighted average: 13.73 +/- 0.04
Forced photometry reference-image weighted average: 13.43 +/- 0.03
Forced photometry reference-image weighted average: 13.50 +/- 0.03
Forced photometry filter REJECTED candidate at 10:38:16.68 +08:24:36.5: ref_mag=13.73 +/- 0.04 new_mean_mag=13.6797 delta=0.05 (need > 0.90)
Forced photometry filter REJECTED candidate at 10:39:45.07 +06:01:51.5: ref_mag=13.43 +/- 0.03 new_mean_mag=13.3461 delta=0.08 (need > 0.90)
Forced photometry on wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 10:55:49.98 +02:33:26.9: 15.80 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 11.23 +/- 0.00
Forced photometry filter REJECTED candidate at 10:51:31.55 +05:28:00.8: ref_mag=13.50 +/- 0.03 new_mean_mag=13.3787 delta=0.12 (need > 0.90)
Forced photometry on wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 10:43:54.36 +05:30:22.7: 15.75 +/- 99.00 upperlimit
Forced photometry filter REJECTED candidate at 11:33:01.22 +09:37:21.4: ref_mag=11.23 +/- 0.00 new_mean_mag=11.3730 delta=-0.14 (need > 0.90)
Forced photometry on wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 11:05:07.70 +02:19:24.5: 15.84 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 10:59:57.23 +04:45:59.7: 15.92 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 11:04:58.18 +07:22:13.4: 13.39 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.41 +/- 0.03
Forced photometry filter REJECTED candidate at 11:04:58.18 +07:22:13.4: ref_mag=13.41 +/- 0.03 new_mean_mag=13.3626 delta=0.05 (need > 0.90)
Forced photometry on wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 10:43:52.89 +05:11:49.7: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 11:05:07.70 +02:19:24.5: 15.82 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q1b1x1_2026-04-19_00-35-13_20.00sec_-4.90C_LIGHT_0503.fits at 10:59:51.57 +08:40:29.3: 15.92 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-07-Q1b1x1_2026-05-10_23-29-38_20.00sec_-4.90C_LIGHT_0148.fits at 10:59:51.57 +08:40:29.3: 15.88 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out32760.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32785.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32973.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33036.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33045.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33046.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 12s
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: 4s
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Considering the candidate 32450_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547
The candidate 32450_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547 did not pass the final checks
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Considering the candidate 32451_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547
The candidate 32451_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547 did not pass the final checks
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Considering the candidate 32453_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547
The candidate 32453_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547 did not pass the final checks
**** FOUND 10:37:35.06 +05:05:25.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32574_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547
The candidate 32574_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547 did not pass the final checks
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Considering the candidate 32666_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547
The candidate 32666_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547 did not pass the final checks
**** FOUND 10:40:59.60 +05:47:49.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32672_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547
The candidate 32672_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547 did not pass the final checks
**** FOUND 10:41:28.23 +08:34:31.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32760_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547
Preparing report for the candidate 32760_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547
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Considering the candidate 32785_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547
Preparing report for the candidate 32785_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547
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Considering the candidate 32841_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547
The candidate 32841_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547 did not pass the final checks
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Considering the candidate 32901_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547
The candidate 32901_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547 did not pass the final checks
**** FOUND 11:21:16.92 +06:01:25.5 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 32908_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547
The candidate 32908_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547 did not pass the final checks
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Considering the candidate 32962_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547
The candidate 32962_fd_Leo-07-Q1b1x1_2026-10-12_06-31-07_20.00sec_0.00C_LIGHTs_0547 did not pass the final checks
