This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB
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 06 02.1370 2461193.6370 12.09 10:47:55.75 +23:48:47.1
212.77367 61.99741 galactic LMi Second-epoch detections are separated by 0.7" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.511 Davida -3 1 3 12.2 0 -0
Forced photometry on wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:55.75 +23:48:47.1: 16.03 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:55.75 +23:48:47.1: 16.01 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461193.6370,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260602.1370 12.09CV 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 06 02.1370 2461193.6370 12.71 10:47:14.17 +20:08:37.6
220.02552 60.79228 galactic Leo Second-epoch detections are separated by 0.3" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.416 Vaticana -3 1 3 12.8 -0 -0
Forced photometry on wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:14.17 +20:08:37.6: 16.20 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:14.17 +20:08:37.6: 16.15 +/- 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 06 02.1370* 10 47 14.17 +20 08 37.6 12.7 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461193.6370,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260602.1370 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 02.1370 2461193.6370 14.21 10:42:18.79 +19:33:01.7
220.34221 59.50104 galactic Leo Second-epoch detections are separated by 1.6" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.508 Princetonia -4 1 4 14.3 0 0
Forced photometry on wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:42:18.79 +19:33:01.7: 16.09 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:42:18.79 +19:33:01.7: 16.09 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 02.1370* 10 42 18.79 +19 33 01.7 14.2 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461193.6370,14.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260602.1370 14.21CV 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 06 02.1370 2461193.6370 14.71 11:05:39.81 +25:06:29.5
211.80234 66.21434 galactic LMi Second-epoch detections are separated by 0.6" and 7.8 pix
The object was found in VSX 1" ST LMi
Type: AM
# Max. Min./Amp. JD0 Period
14.400 V 18.500 V 2459298.42360 0.079089120000 WD+M5-6V
The object was not found in astcheck.
Forced photometry on wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 11:05:39.81 +25:06:29.5: 16.17 +/- 0.34 detection
Forced photometry on wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 11:05:39.81 +25:06:29.5: 16.07 +/- 0.32 detection
Forced photometry reference-image weighted average: 16.12 +/- 0.23
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ST LMi,2461193.6370,14.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ST LMi 20260602.1370 14.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461146.74685282 16.04.2026 05:55:18.084 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
First image: 2461146.74685282 16.04.2026 05:55:18.084 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
Last image: 2461193.63730159 02.06.2026 03:17:32.857 /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.47
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 5645
Objects passed selection criteria: 5640
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 5071.75
Average stars matched: 4990 (98.3881 %)
Memory usage VmPeak: 111704 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Mon Jun 1 15:05:05 CDT 2026
VaST build number 1.0rc89-85-g6dfb2809
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-01)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Jun 1 22:35:30 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: 2461146.74685282 16.04.2026 05:55:18.084 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
First image: 2461146.74685282 16.04.2026 05:55:18.084 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
Last image: 2461193.63730159 02.06.2026 03:17:32.857 /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 17
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.20
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): 29616
Objects passed selection criteria: 29545
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 27208
Average stars matched: 26418 (97.0964 %)
Memory usage VmPeak: 132888 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Mon Jun 1 15:05:05 CDT 2026
VaST build number 1.0rc89-85-g6dfb2809
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-06-01)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Jun 1 22:36:52 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits
SExtractor catalog cache: saved Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat to cache
SExtractor catalog cache: saved Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.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-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.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: 2461193.63671911
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits exists and is non-empty
Saving wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits to local_wcs_cache/
'wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits' -> 'local_wcs_cache/wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits'
wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits exists and is non-empty
Saving wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits to local_wcs_cache/
'wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits' -> 'local_wcs_cache/wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits'
wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits exists and is non-empty
Saving wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits to local_wcs_cache/
'wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits' -> 'local_wcs_cache/wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits'
wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits exists and is non-empty
Saving wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits to local_wcs_cache/
'wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits' -> 'local_wcs_cache/wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits (1st reference image)
verification OK: wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
Image size: 941.3'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:04:39.947 +21:57:23.32 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-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits (1st new image)
verification OK: wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits
Image size: 941.0'x626.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.88"/pix along the Y axis
Image center: 11:04:56.784 +22:01:42.55 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:04:39.947 +21:57:23.32
Second-epoch image center 11:04:56.784 +22:01:42.55
Angular distance between the image centers 0.0970 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits (2nd new image)
verification OK: wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits
Image size: 941.0'x626.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.88"/pix along the Y axis
Image center: 11:04:59.344 +22:02:12.20 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:04:39.947 +21:57:23.32
Second-epoch image center 11:04:59.344 +22:02:12.20
Angular distance between the image centers 0.1098 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 11:04:56.784 +22:01:42.55
Second-epoch second image center 11:04:59.344 +22:02:12.20
Angular distance between the image centers 0.01287 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-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits &> /tmp/tmp.cdkZiJj1sb
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits &> /tmp/tmp.5Bd2JBzaMi
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits &> /tmp/tmp.rrHR1EqJWu
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits &> /tmp/tmp.TkWQgpxIjS
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.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-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits and wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits and wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat
Found non-empty wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits and wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat
The reference image (wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits) and catalog (wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat) found
'wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat' -> 'wcsmag.cat'
Read 5863 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 157.6102 to 175.2048 deg, Dec +16.0221 to +27.5014 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 157.6102 to 175.2048 deg, Dec 16.0221 to 27.5014 deg
Loaded 4338 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): 3191 out of 3323 total matches.
Matched with Tycho-2 3323 out of 5863 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.858500
a=0.000000 b=1.000000 c=22.858500
From vast_summary.log: estimated ref. image limiting mag.: -7.47
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.39
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.39
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 5863 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 157.6102 to 175.2048 deg, Dec +16.0221 to +27.5014 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 157.6102 to 175.2048 deg, Dec 16.0221 to 27.5014 deg
Loaded 4338 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): 3191 out of 3323 total matches.
Matched with Tycho-2 3323 out of 5863 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits:
Forced-photometry filter: calibrated wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits -> calib.txt_param_ref_wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits (aperture=6.2)
Read 5873 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 157.6053 to 175.1804 deg, Dec +16.0221 to +27.5014 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 157.6053 to 175.1804 deg, Dec 16.0221 to 27.5014 deg
Loaded 4338 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): 3172 out of 3318 total matches.
Matched with Tycho-2 3318 out of 5873 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits:
Forced-photometry filter: calibrated wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits -> calib.txt_param_ref_wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
2.1 pix Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
2.5 pix fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits
2.5 pix fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits
2.1 pix wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
2.1 pix wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
Limiting magnitude estimates:
15.4 mag. Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
15.4 mag. Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
14.9 mag. fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits
14.8 mag. fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 12.0 (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.cdkZiJj1sb (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.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-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits' -> 'wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
WCS_IMAGE_NAME=wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
WCS-calibrated image found: wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
Checking if the catalog wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat corresponding to the image wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits alredy exist and is non-empty...
Catalog wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat corresponding to the image wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
WCS catalog name: wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=376, passed=5863
Got 5863 stars (including 5481 good ones) from the SExtractor catalog wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat
util/solve_plate_with_UCAC5 got 5863 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 530 to 589 (Dec 16.0 to 27.5)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 5794 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.0 to 27.5)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 5794 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 5794 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits N_match=944 sigma_overall_arcsec=0.274 sigma_q1_arcsec=0.217 sigma_q2_arcsec=0.328 sigma_q3_arcsec=0.235 sigma_q4_arcsec=0.295 n_q1=218 n_q2=240 n_q3=245 n_q4=241 worst_quadrant_to_overall_ratio=1.200
The image catalog is written to wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits -region wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.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.5Bd2JBzaMi (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.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-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits' -> 'wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
WCS_IMAGE_NAME=wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
WCS-calibrated image found: wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
Checking if the catalog wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.cat corresponding to the image wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits alredy exist and is non-empty...
Catalog wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.cat corresponding to the image wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
WCS catalog name: wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=393, passed=5873
Got 5873 stars (including 5475 good ones) from the SExtractor catalog wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.cat
util/solve_plate_with_UCAC5 got 5873 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 530 to 589 (Dec 16.0 to 27.5)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 5771 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.0 to 27.5)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 5770 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 5770 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits N_match=943 sigma_overall_arcsec=0.310 sigma_q1_arcsec=0.277 sigma_q2_arcsec=0.404 sigma_q3_arcsec=0.269 sigma_q4_arcsec=0.301 n_q1=217 n_q2=238 n_q3=247 n_q4=241 worst_quadrant_to_overall_ratio=1.306
The image catalog is written to wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits -region wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.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.rrHR1EqJWu (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_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.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_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits
WCS_IMAGE_NAME=wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits
WCS-calibrated image found: wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits
Checking if the catalog wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits.cat corresponding to the image wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits.cat corresponding to the image wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits
WCS catalog name: wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=210, passed=4368
Got 4368 stars (including 4150 good ones) from the SExtractor catalog wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits.cat
util/solve_plate_with_UCAC5 got 4368 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 925 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 4323 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 4324 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 4324 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 939 stars left (next iteration limit 1032)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits N_match=939 sigma_overall_arcsec=0.302 sigma_q1_arcsec=0.316 sigma_q2_arcsec=0.302 sigma_q3_arcsec=0.307 sigma_q4_arcsec=0.287 n_q1=230 n_q2=251 n_q3=220 n_q4=238 worst_quadrant_to_overall_ratio=1.047
The image catalog is written to wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits -region wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.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.TkWQgpxIjS (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_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.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_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits
WCS_IMAGE_NAME=wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits
WCS-calibrated image found: wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits
Checking if the catalog wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits.cat corresponding to the image wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits.cat corresponding to the image wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits
WCS catalog name: wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=214, passed=4299
Got 4299 stars (including 4081 good ones) from the SExtractor catalog wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits.cat
util/solve_plate_with_UCAC5 got 4299 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 589 (Dec 16.3 to 27.5)
Done reading UCAC5 zone files...
Matched 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 926 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 4263 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
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 589 (Dec 16.3 to 27.5)
Done reading UCAC5 zone files...
Matched 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 4264 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 4264 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 938 stars left (next iteration limit 1031)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits N_match=938 sigma_overall_arcsec=0.285 sigma_q1_arcsec=0.293 sigma_q2_arcsec=0.316 sigma_q3_arcsec=0.242 sigma_q4_arcsec=0.272 n_q1=232 n_q2=246 n_q3=220 n_q4=240 worst_quadrant_to_overall_ratio=1.108
The image catalog is written to wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits -region wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.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-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits sigma_overall=0.274 worst_q_ratio=1.200
ref2=Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits sigma_overall=0.310 worst_q_ratio=1.306
new1=fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits sigma_overall=0.302 worst_q_ratio=1.047
new2=fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits sigma_overall=0.285 worst_q_ratio=1.108
reference average sigma_overall=0.292 worst_q_ratio=1.253
warn-on-ratio threshold: 2.0x reference
###################################
Distribution of catalog-matched stars across the image:
plot_astrometric_residuals_xy: wrote wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176_astrometric_residuals.png (944 matched stars from wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177_astrometric_residuals.png (943 matched stars from wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044_astrometric_residuals.png (939 matched stars from wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045_astrometric_residuals.png (938 matched stars from wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits.cat.astrometric_residuals, image 9576x6388)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits'
Saving fully-calibrated image wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits'
Preparing the HTML report for the field Leo-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:55.75 +23:48:47.1: 16.03 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:55.75 +23:48:47.1: 16.01 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out20310.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20286_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045
The candidate 20286_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045 did not pass the final checks
**** FOUND 10:56:23.19 +22:21:28.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20310_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045
Preparing report for the candidate 20310_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 7s
Prepared the HTML report for the field Leo-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
10:47:55.75 +23:48:47.1
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits
SExtractor catalog cache: saved Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat to cache
SExtractor catalog cache: saved Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.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-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
Creating symlink local_wcs_cache/wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.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-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits exists and is non-empty
wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits exists and is non-empty
wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits exists and is non-empty
wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits (1st reference image)
verification OK: wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
Image size: 941.3'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 11:04:39.947 +21:57:23.32 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-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits (1st new image)
verification OK: wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits
Image size: 941.0'x626.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.88"/pix along the Y axis
Image center: 11:04:56.784 +22:01:42.55 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:04:39.947 +21:57:23.32
Second-epoch image center 11:04:56.784 +22:01:42.55
Angular distance between the image centers 0.0970 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits (2nd new image)
verification OK: wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits
Image size: 941.0'x626.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.88"/pix along the Y axis
Image center: 11:04:59.344 +22:02:12.20 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:04:39.947 +21:57:23.32
Second-epoch image center 11:04:59.344 +22:02:12.20
Angular distance between the image centers 0.1098 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 11:04:56.784 +22:01:42.55
Second-epoch second image center 11:04:59.344 +22:02:12.20
Angular distance between the image centers 0.01287 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-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits &> /tmp/tmp.DHsg0wdOL0
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits &> /tmp/tmp.iI5vGPsTEt
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits &> /tmp/tmp.Bs5hdM3wDP
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits &> /tmp/tmp.u8tbkW9O5U
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.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-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits and wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits and wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat
Found non-empty wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits and wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat
The reference image (wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits) and catalog (wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat) found
'wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat' -> 'wcsmag.cat'
Read 31701 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 157.6097 to 175.2801 deg, Dec +16.0221 to +27.5078 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 157.6097 to 175.2801 deg, Dec 16.0221 to 27.5078 deg
Loaded 4353 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): 3103 out of 3360 total matches.
Matched with Tycho-2 3360 out of 31701 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.749800
a=0.000000 b=1.000000 c=22.749800
From vast_summary.log: estimated ref. image limiting mag.: -7.20
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.55
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.55
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 31701 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 157.6097 to 175.2801 deg, Dec +16.0221 to +27.5078 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 157.6097 to 175.2801 deg, Dec 16.0221 to 27.5078 deg
Loaded 4353 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): 3103 out of 3360 total matches.
Matched with Tycho-2 3360 out of 31701 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits:
Forced-photometry filter: calibrated wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits -> calib.txt_param_ref_wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits (aperture=4.8)
Read 31604 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 157.5943 to 175.2797 deg, Dec +16.0221 to +27.5110 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 157.5943 to 175.2797 deg, Dec 16.0221 to 27.5110 deg
Loaded 4362 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): 3082 out of 3366 total matches.
Matched with Tycho-2 3366 out of 31604 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits:
Forced-photometry filter: calibrated wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits -> calib.txt_param_ref_wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits (aperture=4.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 17 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
2.0 pix Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
2.4 pix fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits
2.4 pix fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits
2.0 pix wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
2.0 pix wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
Limiting magnitude estimates:
15.6 mag. Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
15.5 mag. Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
14.9 mag. fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits
14.9 mag. fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 14.4 (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.DHsg0wdOL0 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.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-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits' -> 'wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
WCS_IMAGE_NAME=wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
WCS-calibrated image found: wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
Checking if the catalog wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat corresponding to the image wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits alredy exist and is non-empty...
Catalog wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat corresponding to the image wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits
WCS catalog name: wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=1119, passed=31691
Got 31691 stars (including 30518 good ones) from the SExtractor catalog wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat
util/solve_plate_with_UCAC5 got 31691 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 530 to 589 (Dec 16.0 to 27.5)
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 31378 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.0 to 27.5)
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 31379 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 31379 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits N_match=943 sigma_overall_arcsec=0.262 sigma_q1_arcsec=0.216 sigma_q2_arcsec=0.305 sigma_q3_arcsec=0.223 sigma_q4_arcsec=0.282 n_q1=220 n_q2=244 n_q3=242 n_q4=237 worst_quadrant_to_overall_ratio=1.165
The image catalog is written to wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits -region wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.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.iI5vGPsTEt (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.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-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits' -> 'wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
WCS_IMAGE_NAME=wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
WCS-calibrated image found: wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
Checking if the catalog wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.cat corresponding to the image wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits alredy exist and is non-empty...
Catalog wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.cat corresponding to the image wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits
WCS catalog name: wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=1160, passed=31586
Got 31586 stars (including 30372 good ones) from the SExtractor catalog wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.cat
util/solve_plate_with_UCAC5 got 31586 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 530 to 589 (Dec 16.0 to 27.5)
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 31157 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.0 to 27.5)
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 31156 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 31156 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 942 stars left (next iteration limit 1036)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits N_match=942 sigma_overall_arcsec=0.309 sigma_q1_arcsec=0.277 sigma_q2_arcsec=0.375 sigma_q3_arcsec=0.255 sigma_q4_arcsec=0.308 n_q1=219 n_q2=242 n_q3=244 n_q4=237 worst_quadrant_to_overall_ratio=1.214
The image catalog is written to wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits -region wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.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.Bs5hdM3wDP (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_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.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_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits
WCS_IMAGE_NAME=wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits
WCS-calibrated image found: wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits
Checking if the catalog wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits.cat corresponding to the image wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits.cat corresponding to the image wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits
WCS catalog name: wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=583, passed=23190
Got 23190 stars (including 22563 good ones) from the SExtractor catalog wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits.cat
util/solve_plate_with_UCAC5 got 23190 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 22948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 22949 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 22949 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 941 stars left (next iteration limit 1035)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits N_match=941 sigma_overall_arcsec=0.301 sigma_q1_arcsec=0.316 sigma_q2_arcsec=0.319 sigma_q3_arcsec=0.292 sigma_q4_arcsec=0.272 n_q1=229 n_q2=249 n_q3=221 n_q4=242 worst_quadrant_to_overall_ratio=1.060
The image catalog is written to wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits -region wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.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.u8tbkW9O5U (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_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.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_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits
WCS_IMAGE_NAME=wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits
WCS-calibrated image found: wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits
Checking if the catalog wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits.cat corresponding to the image wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits.cat corresponding to the image wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits
WCS catalog name: wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=661, passed=23154
Got 23154 stars (including 22465 good ones) from the SExtractor catalog wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits.cat
util/solve_plate_with_UCAC5 got 23154 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 928 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 22905 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 22906 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 22906 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 940 stars left (next iteration limit 1034)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits N_match=940 sigma_overall_arcsec=0.270 sigma_q1_arcsec=0.288 sigma_q2_arcsec=0.302 sigma_q3_arcsec=0.245 sigma_q4_arcsec=0.251 n_q1=234 n_q2=245 n_q3=220 n_q4=241 worst_quadrant_to_overall_ratio=1.117
The image catalog is written to wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits -region wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.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-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.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_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-16-42_20.00sec_-0.00C_LIGHTs_0044.fits
Saving fully-calibrated image wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.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_2026-06-01_CI_Leo-03-Q1b1x1_223316_TTUQ1b1x1_3811501_jtIxCoJB/wcs_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045.fits
Preparing the HTML report for the field Leo-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 11:33:47.48 +23:24:14.8: 13.17 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:47:14.17 +20:08:37.6: 16.20 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 10:42:18.79 +19:33:01.7: 16.09 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-03-Q1b1x1_2026-04-16_00-55-18_20.00sec_-4.90C_LIGHTs_0176.fits at 11:05:39.81 +25:06:29.5: 16.17 +/- 0.34 detection
Forced photometry on wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 11:33:47.48 +23:24:14.8: 13.14 +/- 0.03 detection
Forced photometry on wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:47:14.17 +20:08:37.6: 16.15 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.15 +/- 0.02
Forced photometry filter REJECTED candidate at 11:33:47.48 +23:24:14.8: ref_mag=13.15 +/- 0.02 new_mean_mag=13.5910 delta=-0.44 (need > 0.90)
Forced photometry on wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 10:42:18.79 +19:33:01.7: 16.09 +/- 99.00 upperlimit
Forced photometry on wcs_Leo-03-Q1b1x1_2026-04-16_00-56-16_20.00sec_-4.90C_LIGHTs_0177.fits at 11:05:39.81 +25:06:29.5: 16.07 +/- 0.32 detection
Forced photometry reference-image weighted average: 16.12 +/- 0.23
Forced photometry filter KEPT candidate at 11:05:39.81 +25:06:29.5: ref_mag=16.12 +/- 0.23 new_mean_mag=14.7017 delta=1.41 (need > 0.90)
Adding exclusion_list_local.txt__out52267.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52419.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52606.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 52241_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045
The candidate 52241_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045 did not pass the final checks
**** FOUND 10:47:55.75 +23:48:46.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52252_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045
The candidate 52252_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045 did not pass the final checks
**** FOUND 10:55:27.49 +24:43:54.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52267_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045
Preparing report for the candidate 52267_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045
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Considering the candidate 52287_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045
The candidate 52287_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045 did not pass the final checks
**** FOUND 11:08:42.05 +24:38:46.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 52295_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045
The candidate 52295_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045 did not pass the final checks
**** FOUND 11:02:28.50 +20:10:47.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 52311_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045
The candidate 52311_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045 did not pass the final checks
**** FOUND 11:13:34.11 +20:06:54.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52312_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045
The candidate 52312_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045 did not pass the final checks
**** FOUND 11:34:40.83 +23:20:03.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52349_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045
The candidate 52349_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045 did not pass the final checks
**** FOUND 10:46:35.71 +24:40:19.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52356_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045
The candidate 52356_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045 did not pass the final checks
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Considering the candidate 52358_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045
The candidate 52358_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045 did not pass the final checks
**** FOUND 11:21:53.41 +19:29:07.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52360_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045
The candidate 52360_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045 did not pass the final checks
**** FOUND 11:21:02.59 +23:49:24.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52374_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045
The candidate 52374_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045 did not pass the final checks
**** FOUND 11:15:01.84 +23:04:41.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52377_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045
The candidate 52377_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045 did not pass the final checks
**** FOUND 11:29:34.03 +18:14:01.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52419_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045
Preparing report for the candidate 52419_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045
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Considering the candidate 52431_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045
The candidate 52431_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045 did not pass the final checks
**** FOUND 11:00:33.44 +23:43:05.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52606_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045
Preparing report for the candidate 52606_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045
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Considering the candidate 20993_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045
The candidate 20993_fd_Leo-03-Q1b1x1_2026-06-01_22-17-32_20.00sec_0.00C_LIGHTs_0045 did not pass the final checks