This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 05 20.1747 2461180.6747 14.65 09:55:10.20 +22:24:00.9
209.70646 49.90628 galactic Leo Second-epoch detections are separated by 1.0" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.567 Eleutheria -5 0 5 14.7 -0 0
Forced photometry on wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits at 09:55:10.20 +22:24:00.9: 16.25 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits at 09:55:10.20 +22:24:00.9: 16.19 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 20.1747* 09 55 10.20 +22 24 00.9 14.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461180.6747,14.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 20260520.1747 14.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 05 20.1747 2461180.6747 14.98 10:09:07.81 +18:03:15.8
217.87223 51.62927 galactic Leo Second-epoch detections are separated by 2.1" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.380 Fiducia -1 1 1 15.2 0 0
Forced photometry on wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits at 10:09:07.81 +18:03:15.8: 16.15 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits at 10:09:07.81 +18:03:15.8: 16.12 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 05 20.1747* 10 09 07.81 +18 03 15.8 15.0 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,2461180.6747,14.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 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 20260520.1747 14.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.85568031 18.01.2026 08:32:00.779 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
First image: 2461058.85568031 18.01.2026 08:32:00.779 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
Last image: 2461180.67500539 20.05.2026 04:11:50.466 /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.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.: -7.44
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: 2 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 6117
Objects passed selection criteria: 6106
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: 4747
Average stars matched: 4425.5 (93.2273 %)
Memory usage VmPeak: 111712 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue May 19 15:05:05 CDT 2026
VaST build number 1.0rc89-63-g0e0f9022
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-19)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue May 19 23:33:26 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.85568031 18.01.2026 08:32:00.779 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
First image: 2461058.85568031 18.01.2026 08:32:00.779 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
Last image: 2461180.67500539 20.05.2026 04:11:50.466 /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 20
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.18
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: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 33930
Objects passed selection criteria: 33815
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: 26676.8
Average stars matched: 24705.2 (92.6097 %)
Memory usage VmPeak: 133928 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue May 19 15:05:05 CDT 2026
VaST build number 1.0rc89-63-g0e0f9022
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-19)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue May 19 23:34:35 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/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits
SExtractor catalog cache: saved Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat to cache
SExtractor catalog cache: saved Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461180.67448459
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
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits exists and is non-empty
Saving wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits to local_wcs_cache/
'wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits' -> 'local_wcs_cache/wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits'
wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits exists and is non-empty
Saving wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits to local_wcs_cache/
'wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits' -> 'local_wcs_cache/wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits'
wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits exists and is non-empty
Saving wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits to local_wcs_cache/
'wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits' -> 'local_wcs_cache/wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits'
wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits exists and is non-empty
Saving wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits to local_wcs_cache/
'wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits' -> 'local_wcs_cache/wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits (1st reference image)
verification OK: wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
Image size: 941.7'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 10:09:14.835 +22:00:04.34 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits (1st new image)
verification OK: wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits
Image size: 937.0'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 10:09:14.011 +22:00:15.46 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 10:09:14.835 +22:00:04.34
Second-epoch image center 10:09:14.011 +22:00:15.46
Angular distance between the image centers 0.0044 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits (2nd new image)
verification OK: wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits
Image size: 937.0'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 10:09:12.537 +21:59:56.62 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 10:09:14.835 +22:00:04.34
Second-epoch image center 10:09:12.537 +21:59:56.62
Angular distance between the image centers 0.0091 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 10:09:14.011 +22:00:15.46
Second-epoch second image center 10:09:12.537 +21:59:56.62
Angular distance between the image centers 0.00773 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits &> /tmp/tmp.b61DoVLHl8
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits &> /tmp/tmp.sptPQM2pSu
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits &> /tmp/tmp.0TEz69mPNe
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits &> /tmp/tmp.fF4gv8rt2V
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits and wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits and wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat
Found non-empty wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits and wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat
The reference image (wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits) and catalog (wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat) found
'wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat' -> 'wcsmag.cat'
Read 6968 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 143.3687 to 160.8868 deg, Dec +16.3927 to +27.3357 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 143.3687 to 160.8868 deg, Dec 16.3927 to 27.3357 deg
Loaded 4674 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3606 out of 3801 total matches.
Matched with Tycho-2 3801 out of 6968 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.899350
a=0.000000 b=1.000000 c=22.899350
From vast_summary.log: estimated ref. image limiting mag.: -7.44
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.46
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.46
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 6968 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 143.3687 to 160.8868 deg, Dec +16.3927 to +27.3357 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 143.3687 to 160.8868 deg, Dec 16.3927 to 27.3357 deg
Loaded 4674 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3606 out of 3801 total matches.
Matched with Tycho-2 3801 out of 6968 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits:
Forced-photometry filter: calibrated wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits -> calib.txt_param_ref_wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits (aperture=6.0)
Read 6793 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 143.3688 to 160.8867 deg, Dec +16.3928 to +27.3358 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 143.3688 to 160.8867 deg, Dec 16.3928 to 27.3358 deg
Loaded 4674 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3603 out of 3798 total matches.
Matched with Tycho-2 3798 out of 6793 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits:
Forced-photometry filter: calibrated wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits -> calib.txt_param_ref_wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits (aperture=6.3)
____ 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: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
2.2 pix Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
2.4 pix fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits
2.3 pix fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits
2.0 pix wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
2.2 pix wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
Limiting magnitude estimates:
15.5 mag. Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
15.4 mag. Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
15.0 mag. fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits
15.0 mag. fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 12.1 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.b61DoVLHl8 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.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_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits' -> 'wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
WCS_IMAGE_NAME=wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
WCS-calibrated image found: wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
Checking if the catalog wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat corresponding to the image wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits alredy exist and is non-empty...
Catalog wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat corresponding to the image wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
WCS catalog name: wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=467, passed=6968
Got 6968 stars (including 6491 good ones) from the SExtractor catalog wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat
util/solve_plate_with_UCAC5 got 6968 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 911 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 910 matched stars entering correct_measured_positions(), 905 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 910 matched stars entering correct_measured_positions(), 6899 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 911 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 910 matched stars entering correct_measured_positions(), 6898 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 910 matched stars entering correct_measured_positions(), 6898 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 910 stars left (next iteration limit 1001)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits N_match=910 sigma_overall_arcsec=0.315 sigma_q1_arcsec=0.375 sigma_q2_arcsec=0.339 sigma_q3_arcsec=0.314 sigma_q4_arcsec=0.259 n_q1=243 n_q2=222 n_q3=230 n_q4=215 worst_quadrant_to_overall_ratio=1.188
The image catalog is written to wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits -region wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.sptPQM2pSu (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.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_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits' -> 'wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
WCS_IMAGE_NAME=wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
WCS-calibrated image found: wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
Checking if the catalog wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits.cat corresponding to the image wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits alredy exist and is non-empty...
Catalog wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits.cat corresponding to the image wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
WCS catalog name: wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=460, passed=6793
Got 6793 stars (including 6327 good ones) from the SExtractor catalog wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits.cat
util/solve_plate_with_UCAC5 got 6793 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 909 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 908 matched stars entering correct_measured_positions(), 904 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 908 matched stars entering correct_measured_positions(), 6708 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 909 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 908 matched stars entering correct_measured_positions(), 6707 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 908 matched stars entering correct_measured_positions(), 6707 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 908 stars left (next iteration limit 998)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits N_match=908 sigma_overall_arcsec=0.372 sigma_q1_arcsec=0.444 sigma_q2_arcsec=0.339 sigma_q3_arcsec=0.338 sigma_q4_arcsec=0.366 n_q1=243 n_q2=222 n_q3=231 n_q4=212 worst_quadrant_to_overall_ratio=1.191
The image catalog is written to wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits -region wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.0TEz69mPNe (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits
WCS_IMAGE_NAME=wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits
WCS-calibrated image found: wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits
Checking if the catalog wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits.cat corresponding to the image wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits.cat corresponding to the image wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits
WCS catalog name: wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=337, passed=5415
Got 5415 stars (including 5073 good ones) from the SExtractor catalog wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits.cat
util/solve_plate_with_UCAC5 got 5415 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 901 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 901 matched stars entering correct_measured_positions(), 888 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 901 matched stars entering correct_measured_positions(), 5327 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 901 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 901 matched stars entering correct_measured_positions(), 5328 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 901 matched stars entering correct_measured_positions(), 5328 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 901 stars left (next iteration limit 991)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits N_match=901 sigma_overall_arcsec=0.466 sigma_q1_arcsec=0.318 sigma_q2_arcsec=0.718 sigma_q3_arcsec=0.369 sigma_q4_arcsec=0.525 n_q1=215 n_q2=232 n_q3=189 n_q4=265 worst_quadrant_to_overall_ratio=1.539
The image catalog is written to wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits -region wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.fF4gv8rt2V (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits
WCS_IMAGE_NAME=wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits
WCS-calibrated image found: wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits
Checking if the catalog wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits.cat corresponding to the image wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits.cat corresponding to the image wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits
WCS catalog name: wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=357, passed=5389
Got 5389 stars (including 5027 good ones) from the SExtractor catalog wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits.cat
util/solve_plate_with_UCAC5 got 5389 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 903 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 902 matched stars entering correct_measured_positions(), 894 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 902 matched stars entering correct_measured_positions(), 5296 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 903 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 902 matched stars entering correct_measured_positions(), 5297 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 902 matched stars entering correct_measured_positions(), 5297 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 902 stars left (next iteration limit 992)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits N_match=902 sigma_overall_arcsec=0.486 sigma_q1_arcsec=0.343 sigma_q2_arcsec=0.775 sigma_q3_arcsec=0.377 sigma_q4_arcsec=0.521 n_q1=211 n_q2=234 n_q3=190 n_q4=267 worst_quadrant_to_overall_ratio=1.594
The image catalog is written to wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits -region wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits sigma_overall=0.315 worst_q_ratio=1.188
ref2=Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits sigma_overall=0.372 worst_q_ratio=1.191
new1=fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits sigma_overall=0.466 worst_q_ratio=1.539
new2=fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits sigma_overall=0.486 worst_q_ratio=1.594
reference average sigma_overall=0.3435 worst_q_ratio=1.1895
warn-on-ratio threshold: 2.0x reference
###################################
Distribution of catalog-matched stars across the image:
plot_astrometric_residuals_xy: wrote wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380_astrometric_residuals.png (910 matched stars from wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225_astrometric_residuals.png (908 matched stars from wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112_astrometric_residuals.png (901 matched stars from wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113_astrometric_residuals.png (902 matched stars from wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits.cat.astrometric_residuals, image 9576x6388)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits'
Saving fully-calibrated image wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits'
Preparing the HTML report for the field Leo-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Leo-02-Q2b1x1 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 --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits
SExtractor catalog cache: saved Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat to cache
SExtractor catalog cache: saved Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
Creating symlink local_wcs_cache/wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits exists and is non-empty
wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits exists and is non-empty
wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits exists and is non-empty
wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits (1st reference image)
verification OK: wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
Image size: 941.7'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 10:09:14.835 +22:00:04.34 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits (1st new image)
verification OK: wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits
Image size: 937.0'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 10:09:14.011 +22:00:15.46 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 10:09:14.835 +22:00:04.34
Second-epoch image center 10:09:14.011 +22:00:15.46
Angular distance between the image centers 0.0044 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits (2nd new image)
verification OK: wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits
Image size: 937.0'x624.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 10:09:12.537 +21:59:56.62 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 10:09:14.835 +22:00:04.34
Second-epoch image center 10:09:12.537 +21:59:56.62
Angular distance between the image centers 0.0091 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 10:09:14.011 +22:00:15.46
Second-epoch second image center 10:09:12.537 +21:59:56.62
Angular distance between the image centers 0.00773 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits &> /tmp/tmp.yYjyJTQRcn
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits &> /tmp/tmp.PQlIQS3yYV
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits &> /tmp/tmp.2vyFkFfVa6
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits &> /tmp/tmp.cEGr9mA1iO
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits and wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits and wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat
Found non-empty wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits and wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat
The reference image (wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits) and catalog (wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat) found
'wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat' -> 'wcsmag.cat'
Read 37822 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 143.3687 to 160.9043 deg, Dec +16.3249 to +27.3468 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 143.3687 to 160.9043 deg, Dec 16.3249 to 27.3468 deg
Loaded 4718 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3458 out of 3819 total matches.
Matched with Tycho-2 3819 out of 37822 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.797900
a=0.000000 b=1.000000 c=22.797900
From vast_summary.log: estimated ref. image limiting mag.: -7.18
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.62
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.62
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 37822 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 143.3687 to 160.9043 deg, Dec +16.3249 to +27.3468 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 143.3687 to 160.9043 deg, Dec 16.3249 to 27.3468 deg
Loaded 4718 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3458 out of 3819 total matches.
Matched with Tycho-2 3819 out of 37822 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits:
Forced-photometry filter: calibrated wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits -> calib.txt_param_ref_wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits (aperture=4.8)
Read 36566 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 143.3688 to 160.9045 deg, Dec +16.3177 to +27.3431 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 143.3688 to 160.9045 deg, Dec 16.3177 to 27.3431 deg
Loaded 4721 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3449 out of 3818 total matches.
Matched with Tycho-2 3818 out of 36566 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits:
Forced-photometry filter: calibrated wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits -> calib.txt_param_ref_wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits (aperture=4.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 18 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
1.9 pix Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
2.1 pix Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
2.2 pix fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits
2.2 pix fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits
1.9 pix wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
2.1 pix wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
Limiting magnitude estimates:
15.6 mag. Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
15.5 mag. Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
15.1 mag. fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits
15.1 mag. fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 14.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.yYjyJTQRcn (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.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_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits' -> 'wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
WCS_IMAGE_NAME=wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
WCS-calibrated image found: wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
Checking if the catalog wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat corresponding to the image wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits alredy exist and is non-empty...
Catalog wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat corresponding to the image wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits
WCS catalog name: wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=1597, passed=37808
Got 37808 stars (including 36133 good ones) from the SExtractor catalog wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat
util/solve_plate_with_UCAC5 got 37808 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 903 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 902 matched stars entering correct_measured_positions(), 896 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 902 matched stars entering correct_measured_positions(), 37316 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 903 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 902 matched stars entering correct_measured_positions(), 37317 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 902 matched stars entering correct_measured_positions(), 37317 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 902 stars left (next iteration limit 992)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits N_match=902 sigma_overall_arcsec=0.317 sigma_q1_arcsec=0.342 sigma_q2_arcsec=0.330 sigma_q3_arcsec=0.332 sigma_q4_arcsec=0.251 n_q1=244 n_q2=222 n_q3=229 n_q4=207 worst_quadrant_to_overall_ratio=1.077
The image catalog is written to wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits -region wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.PQlIQS3yYV (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.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_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits' -> 'wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
WCS_IMAGE_NAME=wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
WCS-calibrated image found: wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
Checking if the catalog wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits.cat corresponding to the image wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits alredy exist and is non-empty...
Catalog wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits.cat corresponding to the image wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits
WCS catalog name: wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=1590, passed=36553
Got 36553 stars (including 34890 good ones) from the SExtractor catalog wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits.cat
util/solve_plate_with_UCAC5 got 36553 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 903 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 902 matched stars entering correct_measured_positions(), 896 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 902 matched stars entering correct_measured_positions(), 36060 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
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 903 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 902 matched stars entering correct_measured_positions(), 36061 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 902 matched stars entering correct_measured_positions(), 36061 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 902 stars left (next iteration limit 992)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits N_match=902 sigma_overall_arcsec=0.360 sigma_q1_arcsec=0.410 sigma_q2_arcsec=0.332 sigma_q3_arcsec=0.343 sigma_q4_arcsec=0.340 n_q1=243 n_q2=220 n_q3=229 n_q4=210 worst_quadrant_to_overall_ratio=1.140
The image catalog is written to wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits -region wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.2vyFkFfVa6 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits
WCS_IMAGE_NAME=wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits
WCS-calibrated image found: wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits
Checking if the catalog wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits.cat corresponding to the image wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits.cat corresponding to the image wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits
WCS catalog name: wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=1361, passed=27845
Got 27845 stars (including 26460 good ones) from the SExtractor catalog wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits.cat
util/solve_plate_with_UCAC5 got 27845 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 899 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 899 matched stars entering correct_measured_positions(), 887 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 899 matched stars entering correct_measured_positions(), 27352 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 899 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 899 matched stars entering correct_measured_positions(), 27353 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 899 matched stars entering correct_measured_positions(), 27353 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 899 stars left (next iteration limit 988)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits N_match=899 sigma_overall_arcsec=0.465 sigma_q1_arcsec=0.299 sigma_q2_arcsec=0.721 sigma_q3_arcsec=0.369 sigma_q4_arcsec=0.492 n_q1=213 n_q2=221 n_q3=205 n_q4=260 worst_quadrant_to_overall_ratio=1.552
The image catalog is written to wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits -region wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.cEGr9mA1iO (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits
WCS_IMAGE_NAME=wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits
WCS-calibrated image found: wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits
Checking if the catalog wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits.cat corresponding to the image wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits.cat corresponding to the image wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits
WCS catalog name: wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=1479, passed=28003
Got 28003 stars (including 26483 good ones) from the SExtractor catalog wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits.cat
util/solve_plate_with_UCAC5 got 28003 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 898 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 898 matched stars entering correct_measured_positions(), 887 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 898 matched stars entering correct_measured_positions(), 27454 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.6 to 27.3)
Done reading UCAC5 zone files...
Matched 898 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 898 matched stars entering correct_measured_positions(), 27454 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 898 matched stars entering correct_measured_positions(), 27454 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 898 stars left (next iteration limit 987)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits N_match=898 sigma_overall_arcsec=0.492 sigma_q1_arcsec=0.330 sigma_q2_arcsec=0.697 sigma_q3_arcsec=0.397 sigma_q4_arcsec=0.515 n_q1=210 n_q2=222 n_q3=205 n_q4=261 worst_quadrant_to_overall_ratio=1.417
The image catalog is written to wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits -region wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-05_20.00sec_4.90C_LIGHT_0112.fits
Saving fully-calibrated image wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-05-19_CI_Leo-02-Q2b1x1_233112_TTUQ2b1x1_737581_mzr75n6F/wcs_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113.fits
Preparing the HTML report for the field Leo-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits at 10:23:33.61 +20:17:09.0: 14.94 +/- 0.11 detection
Forced photometry on wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits at 10:02:33.95 +24:05:02.3: 14.32 +/- 0.06 detection
Forced photometry on wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits at 10:16:46.38 +23:01:15.8: 13.21 +/- 0.02 detection
Forced photometry on wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits at 10:21:46.08 +21:23:04.5: 14.26 +/- 0.07 detection
Forced photometry on wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits at 10:06:37.32 +17:54:42.9: 14.27 +/- 0.08 detection
Forced photometry on wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits at 10:09:07.81 +18:03:15.8: 16.15 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits at 09:55:10.20 +22:24:00.9: 16.25 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q2b1x1_2026-01-18_02-32-00_20.00sec_-15.00C_LIGHT_0380.fits at 10:11:21.74 +17:45:10.1: 14.29 +/- 0.07 detection
Forced photometry on wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits at 10:02:33.95 +24:05:02.3: 14.34 +/- 0.06 detection
Forced photometry on wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits at 10:16:46.38 +23:01:15.8: 13.18 +/- 0.02 detection
Forced photometry on wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits at 10:23:33.61 +20:17:09.0: 14.93 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.33 +/- 0.04
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Forced photometry filter REJECTED candidate at 10:02:33.95 +24:05:02.3: ref_mag=14.33 +/- 0.04 new_mean_mag=14.3869 delta=-0.06 (need > 0.90)
Forced photometry filter REJECTED candidate at 10:16:46.38 +23:01:15.8: ref_mag=13.19 +/- 0.02 new_mean_mag=13.7221 delta=-0.53 (need > 0.90)
Forced photometry reference-image weighted average: 14.94 +/- 0.08
Forced photometry filter REJECTED candidate at 10:23:33.61 +20:17:09.0: ref_mag=14.94 +/- 0.08 new_mean_mag=14.7460 delta=0.19 (need > 0.90)
Forced photometry on wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits at 10:21:46.08 +21:23:04.5: 14.31 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.28 +/- 0.05
Forced photometry filter REJECTED candidate at 10:21:46.08 +21:23:04.5: ref_mag=14.28 +/- 0.05 new_mean_mag=14.2009 delta=0.08 (need > 0.90)
Forced photometry on wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits at 09:55:10.20 +22:24:00.9: 16.19 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits at 10:09:07.81 +18:03:15.8: 16.12 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits at 10:11:21.74 +17:45:10.1: 14.31 +/- 0.07 detection
Forced photometry on wcs_Leo-02-Q2b1x1_2026-02-21_23-36-27_20.00sec_-15.00C_LIGHT_0225.fits at 10:06:37.32 +17:54:42.9: 14.18 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.22 +/- 0.05
Forced photometry reference-image weighted average: 14.30 +/- 0.05
Forced photometry filter REJECTED candidate at 10:06:37.32 +17:54:42.9: ref_mag=14.22 +/- 0.05 new_mean_mag=14.0865 delta=0.14 (need > 0.90)
Forced photometry filter REJECTED candidate at 10:11:21.74 +17:45:10.1: ref_mag=14.30 +/- 0.05 new_mean_mag=14.4502 delta=-0.15 (need > 0.90)
Adding exclusion_list_local.txt__out56036.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57090.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 51444_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113
The candidate 51444_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113 did not pass the final checks
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Considering the candidate 51447_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113
The candidate 51447_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113 did not pass the final checks
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Considering the candidate 52886_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113
The candidate 52886_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113 did not pass the final checks
**** FOUND 10:23:52.02 +19:34:29.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52906_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113
The candidate 52906_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113 did not pass the final checks
**** FOUND 09:51:55.77 +24:21:46.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 52953_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113
The candidate 52953_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113 did not pass the final checks
**** FOUND 10:26:52.49 +19:22:41.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 53728_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113
The candidate 53728_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113 did not pass the final checks
**** FOUND 09:51:44.29 +20:10:33.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53914_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113
The candidate 53914_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113 did not pass the final checks
**** FOUND 10:19:38.89 +22:31:49.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54035_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113
The candidate 54035_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113 did not pass the final checks
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Considering the candidate 54141_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113
The candidate 54141_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113 did not pass the final checks
**** FOUND 09:50:55.88 +20:47:14.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54248_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113
The candidate 54248_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113 did not pass the final checks
**** FOUND 09:59:30.70 +21:18:02.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54816_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113
The candidate 54816_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113 did not pass the final checks
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Considering the candidate 54911_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113
The candidate 54911_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113 did not pass the final checks
**** FOUND 10:06:02.36 +23:50:18.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55185_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113
The candidate 55185_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113 did not pass the final checks
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Considering the candidate 55597_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113
The candidate 55597_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113 did not pass the final checks
**** FOUND 10:14:17.99 +20:25:41.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55705_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113
The candidate 55705_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113 did not pass the final checks
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Considering the candidate 56036_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113
Preparing report for the candidate 56036_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113
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Considering the candidate 57090_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113
Preparing report for the candidate 57090_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113
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Considering the candidate 05152_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113
The candidate 05152_fd_Leo-02-Q2b1x1_2026-05-19_23-11-50_20.00sec_5.00C_LIGHT_0113 did not pass the final checks