This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
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 04 14.2059* 11 13 14.37 +01 30 07.5 12.5 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461144.7059,12.46,0.05,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 20260414.2059 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 14.2059* 11 03 01.54 +02 42 36.7 13.2 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,2461144.7059,13.20,0.05,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 20260414.2059 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 14.2059* 10 40 30.32 +00 30 08.8 13.7 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461144.7059,13.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260414.2059 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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 04 14.2059* 10 43 59.46 -04 36 30.6 14.4 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461144.7059,14.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260414.2059 14.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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 04 14.2059* 11 28 13.22 -06 39 52.4 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,2461144.7059,14.24,0.05,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 20260414.2059 14.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 14.2059* 11 28 32.74 +01 45 35.5 14.5 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461144.7059,14.54,0.05,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 20260414.2059 14.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.90639640 18.01.2026 09:45:02.649 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
First image: 2461058.90639640 18.01.2026 09:45:02.649 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
Last image: 2461144.70625385 14.04.2026 04:56:50.333 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 7
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.68
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): 6424
Objects passed selection criteria: 6415
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 5977.5
Average stars matched: 5816 (97.2982 %)
Memory usage VmPeak: 112176 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Apr 14 00:00:27 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.90639640 18.01.2026 09:45:02.649 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
First image: 2461058.90639640 18.01.2026 09:45:02.649 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
Last image: 2461144.70625385 14.04.2026 04:56:50.333 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 57
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.45
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: 13 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): 33597
Objects passed selection criteria: 33538
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 31554.8
Average stars matched: 30591.8 (96.9482 %)
Memory usage VmPeak: 134724 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Apr 14 00:01:17 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-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits
SExtractor catalog cache: saved Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat to cache
SExtractor catalog cache: saved Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.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-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.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: 2461144.70545872
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
'tns_transients_list.txt' -> '../tns_transients_list.txt'
wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits exists and is non-empty
Saving wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits to local_wcs_cache/
'wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits' -> 'local_wcs_cache/wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits'
wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits exists and is non-empty
Saving wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits to local_wcs_cache/
'wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits' -> 'local_wcs_cache/wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits'
wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits exists and is non-empty
Saving wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits to local_wcs_cache/
'wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits' -> 'local_wcs_cache/wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits'
wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits exists and is non-empty
Saving wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits to local_wcs_cache/
'wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits' -> 'local_wcs_cache/wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:08:34.742 -01:59:53.74
Second-epoch image center 11:08:37.957 -01:56:42.97
Angular distance between the image centers 0.0547 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:08:34.742 -01:59:53.74
Second-epoch image center 11:08:38.170 -01:57:33.86
Angular distance between the image centers 0.0414 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 11:08:37.957 -01:56:42.97
Second-epoch second image center 11:08:38.170 -01:57:33.86
Angular distance between the image centers 0.01416 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-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits &> /tmp/tmp.CWWA9pXVyK
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits &> /tmp/tmp.fixxIZYcUb
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits &> /tmp/tmp.F3IOchPqwy
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits &> /tmp/tmp.gTpU7N8GLj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.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-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits and wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits and wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
Found non-empty wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits and wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
The reference image (wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits) and catalog (wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat) found
'wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat' -> 'wcsmag.cat'
Read 6399 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 159.2436 to 175.0501 deg, Dec -7.2952 to +3.3133 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 159.2436 to 175.0501 deg, Dec -7.2952 to 3.3133 deg
Loaded 3835 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): 3238 out of 3372 total matches.
Matched with Tycho-2 3372 out of 6399 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.879752
a=0.000000 b=1.000000 c=22.879752
From vast_summary.log: estimated ref. image limiting mag.: -7.68
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.20
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.20
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
2.2 pix Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
2.4 pix fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits
2.2 pix fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits
Limiting magnitude estimates:
15.2 mag. Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
15.2 mag. Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
14.9 mag. fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits
15.0 mag. fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits
All-image limiting magnitude estimate: 14.9 (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.CWWA9pXVyK (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_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.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-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits' -> 'wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
WCS_IMAGE_NAME=wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
WCS-calibrated image found: wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
Checking if the catalog wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat corresponding to the image wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits alredy exist and is non-empty...
Catalog wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat corresponding to the image wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
WCS catalog name: wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=432, passed=6399
Got 6399 stars (including 5960 good ones) from the SExtractor catalog wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
util/solve_plate_with_UCAC5 got 6399 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 941 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 6330 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 6329 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 6329 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 947 stars left (next iteration limit 1041)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits -region wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.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.fixxIZYcUb (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_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.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-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits' -> 'wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
WCS_IMAGE_NAME=wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
WCS-calibrated image found: wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
Checking if the catalog wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat corresponding to the image wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits alredy exist and is non-empty...
Catalog wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat corresponding to the image wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
WCS catalog name: wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=407, passed=6519
Got 6519 stars (including 6107 good ones) from the SExtractor catalog wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat
util/solve_plate_with_UCAC5 got 6519 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
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(), 934 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 6416 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
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(), 6418 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 942 matched stars entering correct_measured_positions(), 6418 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 942 stars left (next iteration limit 1036)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits -region wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.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.F3IOchPqwy (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_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.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_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits
WCS_IMAGE_NAME=wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits
WCS-calibrated image found: wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits
Checking if the catalog wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits.cat corresponding to the image wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits.cat corresponding to the image wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits
WCS catalog name: wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=336, passed=5679
Got 5679 stars (including 5335 good ones) from the SExtractor catalog wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits.cat
util/solve_plate_with_UCAC5 got 5679 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (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 411 to 470 (Dec -7.7 to 3.8)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 939 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 5617 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 411 to 470 (Dec -7.7 to 3.8)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 5617 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 5617 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 946 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits -region wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.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.gTpU7N8GLj (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_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.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_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits
WCS_IMAGE_NAME=wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits
WCS-calibrated image found: wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits
Checking if the catalog wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits.cat corresponding to the image wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits.cat corresponding to the image wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits
WCS catalog name: wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=353, passed=5516
Got 5516 stars (including 5155 good ones) from the SExtractor catalog wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits.cat
util/solve_plate_with_UCAC5 got 5516 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (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 411 to 470 (Dec -7.7 to 3.8)
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(), 937 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(), 5465 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 411 to 470 (Dec -7.7 to 3.8)
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(), 5462 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 5462 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits -region wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits'
Saving fully-calibrated image wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits'
Saving fully-calibrated image wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits'
Saving fully-calibrated image wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits'
Preparing the HTML report for the field Leo-08-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
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 20415_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
The candidate 20415_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144 did not pass the final checks
**** FOUND 11:39:48.46 +02:33:51.1 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Leo-08-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits
SExtractor catalog cache: saved Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat to cache
SExtractor catalog cache: saved Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.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-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
Creating symlink local_wcs_cache/wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.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-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits exists and is non-empty
wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits exists and is non-empty
wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits exists and is non-empty
wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:08:34.742 -01:59:53.74
Second-epoch image center 11:08:37.957 -01:56:42.97
Angular distance between the image centers 0.0547 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 11:08:34.742 -01:59:53.74
Second-epoch image center 11:08:38.170 -01:57:33.86
Angular distance between the image centers 0.0414 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 11:08:37.957 -01:56:42.97
Second-epoch second image center 11:08:38.170 -01:57:33.86
Angular distance between the image centers 0.01416 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-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits &> /tmp/tmp.ieb66fDDvK
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits &> /tmp/tmp.hYO6riZJoj
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits &> /tmp/tmp.ZQmqOs21oM
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits &> /tmp/tmp.sf1V3OcGZN
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.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-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits and wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits and wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
Found non-empty wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits and wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
The reference image (wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits) and catalog (wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat) found
'wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat' -> 'wcsmag.cat'
Read 34371 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 159.2400 to 175.0938 deg, Dec -7.3026 to +3.3144 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 159.2400 to 175.0938 deg, Dec -7.3026 to 3.3144 deg
Loaded 3852 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): 3086 out of 3398 total matches.
Matched with Tycho-2 3398 out of 34371 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.774901
a=0.000000 b=1.000000 c=22.774901
From vast_summary.log: estimated ref. image limiting mag.: -7.45
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.32
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.32
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 44 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
2.2 pix Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
2.4 pix fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits
2.1 pix fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits
Limiting magnitude estimates:
15.3 mag. Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
15.3 mag. Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
15.1 mag. fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits
15.1 mag. fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits
All-image limiting magnitude estimate: 15.1 (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.ieb66fDDvK (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_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.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-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits' -> 'wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
WCS_IMAGE_NAME=wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
WCS-calibrated image found: wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
Checking if the catalog wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat corresponding to the image wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits alredy exist and is non-empty...
Catalog wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat corresponding to the image wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
WCS catalog name: wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=1404, passed=34365
Got 34365 stars (including 32904 good ones) from the SExtractor catalog wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat
util/solve_plate_with_UCAC5 got 34365 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
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: 944 matched stars entering correct_measured_positions(), 935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 33882 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
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: 944 matched stars entering correct_measured_positions(), 33882 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 33882 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits -region wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.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.hYO6riZJoj (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_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.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-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits' -> 'wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
WCS_IMAGE_NAME=wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
WCS-calibrated image found: wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
Checking if the catalog wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat corresponding to the image wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits alredy exist and is non-empty...
Catalog wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat corresponding to the image wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
WCS catalog name: wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=1420, passed=33111
Got 33111 stars (including 31640 good ones) from the SExtractor catalog wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat
util/solve_plate_with_UCAC5 got 33111 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
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: 944 matched stars entering correct_measured_positions(), 938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 32671 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
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: 944 matched stars entering correct_measured_positions(), 32673 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 32673 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits -region wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.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.ZQmqOs21oM (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_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.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_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits
WCS_IMAGE_NAME=wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits
WCS-calibrated image found: wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits
Checking if the catalog wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits.cat corresponding to the image wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits.cat corresponding to the image wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits
WCS catalog name: wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=1095, passed=29073
Got 29073 stars (including 27945 good ones) from the SExtractor catalog wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits.cat
util/solve_plate_with_UCAC5 got 29073 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (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 411 to 471 (Dec -7.7 to 3.8)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 936 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 28787 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 411 to 471 (Dec -7.7 to 3.8)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 28788 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 28788 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 947 stars left (next iteration limit 1041)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits -region wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.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.sf1V3OcGZN (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_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.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_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits
WCS_IMAGE_NAME=wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits
WCS-calibrated image found: wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits
Checking if the catalog wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits.cat corresponding to the image wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits.cat corresponding to the image wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits
WCS catalog name: wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=1178, passed=30685
Got 30685 stars (including 29457 good ones) from the SExtractor catalog wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits.cat
util/solve_plate_with_UCAC5 got 30685 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (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 411 to 471 (Dec -7.7 to 3.8)
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(), 934 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(), 30419 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 471 (Dec -7.7 to 3.8)
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(), 30420 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 30420 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits -region wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.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_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/wcs_Leo-08-Q1b1x1_2026-01-18_03-45-02_20.00sec_-14.90C_LIGHT_0455.fits
Saving fully-calibrated image wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.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_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/wcs_Leo-08-Q1b1x1_2026-01-18_03-45-37_20.00sec_-15.00C_LIGHT_0456.fits
Saving fully-calibrated image wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.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_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-55-41_20.00sec_-5.00C_LIGHTs_0143.fits
Saving fully-calibrated image wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.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_2026-04-13_CI_Leo-08-Q1b1x1_235746_TTUQ1b1x1_10145_P17sEWgy/wcs_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144.fits
Preparing the HTML report for the field Leo-08-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out51715.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52091.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52163.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52434.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52548.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52576.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52586.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52659.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52766.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52784.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52817.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52847.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52854.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52857.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out51986.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52153.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52347.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52687.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52691.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52818.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 9s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51712_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
The candidate 51712_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144 did not pass the final checks
**** FOUND 11:35:30.19 +02:10:07.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51715_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
The candidate 51715_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144 did not pass the final checks
**** FOUND 10:38:10.52 -06:19:55.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 0.865 3776569691175536512 159.54402120902 -06.33215119884 12.5178 11.8617 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.865#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51759_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
The candidate 51759_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144 did not pass the final checks
**** FOUND 11:39:48.45 +02:33:51.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51871_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
The candidate 51871_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144 did not pass the final checks
**** FOUND 11:38:33.89 +02:29:51.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51986_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
Preparing report for the candidate 51986_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52015_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
The candidate 52015_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144 did not pass the final checks
**** FOUND 11:38:33.59 +02:30:21.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52091_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
The candidate 52091_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144 did not pass the final checks
**** FOUND 10:51:21.71 +02:00:15.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 1.225 3808319742990503680 162.84077167712 +02.00408873428 13.0845 12.4899 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.225#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52126_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
The candidate 52126_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144 did not pass the final checks
**** FOUND 11:39:31.35 +02:14:44.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52153_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
Preparing report for the candidate 52153_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
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Considering the candidate 52163_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
The candidate 52163_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144 did not pass the final checks
**** FOUND 10:37:13.85 -06:18:02.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 1.346 3776572886631204480 159.30808324671 -06.30058567045 12.9896 12.4505 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.346#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52200_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
The candidate 52200_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144 did not pass the final checks
**** FOUND 11:29:07.33 -02:53:47.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52210_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
The candidate 52210_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144 did not pass the final checks
**** FOUND 11:39:24.08 +02:04:47.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52234_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
The candidate 52234_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144 did not pass the final checks
**** FOUND 11:24:33.41 +00:11:56.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52299_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
The candidate 52299_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144 did not pass the final checks
**** FOUND 11:05:57.99 -05:23:35.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52316_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
The candidate 52316_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144 did not pass the final checks
**** FOUND 11:14:03.17 +02:50:13.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52337_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
The candidate 52337_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144 did not pass the final checks
**** FOUND 10:37:41.27 -03:54:21.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52347_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
Preparing report for the candidate 52347_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
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Considering the candidate 52391_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
The candidate 52391_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144 did not pass the final checks
**** FOUND 11:38:40.89 +02:23:50.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52417_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
The candidate 52417_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144 did not pass the final checks
**** FOUND 10:51:36.89 -02:35:52.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52434_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
The candidate 52434_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144 did not pass the final checks
**** FOUND 11:38:36.84 +01:57:00.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 1.399 3799275400858668160 174.65388876109 +01.95010185029 13.8601 13.3855 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.399#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52437_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
The candidate 52437_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144 did not pass the final checks
**** FOUND 11:39:54.78 +00:59:18.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52452_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
The candidate 52452_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144 did not pass the final checks
**** FOUND 11:38:32.66 +02:34:40.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52516_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
The candidate 52516_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144 did not pass the final checks
**** FOUND 11:39:39.93 +02:11:12.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52548_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
The candidate 52548_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144 did not pass the final checks
**** FOUND 11:37:42.49 +02:27:27.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 0.937 3800475895757525248 174.42730158377 +02.45756467981 13.9806 13.4476 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.937#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52573_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
The candidate 52573_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144 did not pass the final checks
**** FOUND 11:26:50.75 +01:39:50.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52576_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
The candidate 52576_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144 did not pass the final checks
**** FOUND 11:38:21.56 +02:13:46.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 1.184 3799706684294427776 174.59011337702 +02.22927174888 14.1159 13.5148 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.184#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52586_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
The candidate 52586_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144 did not pass the final checks
**** FOUND 11:38:38.68 +02:10:25.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 0.427 3799702561125823104 174.66128533811 +02.17371996319 13.8687 13.4554 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.427#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52608_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
The candidate 52608_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144 did not pass the final checks
**** FOUND 11:39:49.02 +02:21:04.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52623_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
The candidate 52623_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144 did not pass the final checks
**** FOUND 11:39:28.19 +01:49:34.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52644_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
The candidate 52644_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144 did not pass the final checks
**** FOUND 10:55:22.97 +03:14:13.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52659_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
The candidate 52659_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144 did not pass the final checks
**** FOUND 11:38:51.42 +02:27:23.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 1.056 3799728743246466944 174.71453237799 +02.45630819707 14.4219 13.8946 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.056#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52687_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
Preparing report for the candidate 52687_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
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Considering the candidate 52690_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
The candidate 52690_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144 did not pass the final checks
**** FOUND 11:39:42.65 +01:57:30.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52691_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
Preparing report for the candidate 52691_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
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Considering the candidate 52749_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
The candidate 52749_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144 did not pass the final checks
**** FOUND 11:28:57.66 -06:48:32.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52766_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
The candidate 52766_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144 did not pass the final checks
**** FOUND 10:40:50.00 +02:04:56.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.71, MAG_FAINT_SEARCH_LIMIT=15.69)GAIADR2_OUTPUT=# 1.314 3807779333025244544 160.20869852732 +02.08233474025 14.7233 14.2479 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.314#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52784_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
The candidate 52784_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144 did not pass the final checks
**** FOUND 11:23:53.26 +02:44:27.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.55, MAG_FAINT_SEARCH_LIMIT=15.53)GAIADR2_OUTPUT=# 1.982 3810871091003270144 170.97224270184 +02.74138823813 14.5927 13.9404 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.982#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52807_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
The candidate 52807_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144 did not pass the final checks
**** FOUND 11:16:40.45 +02:49:06.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52817_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
The candidate 52817_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144 did not pass the final checks
**** FOUND 11:27:25.60 -03:25:23.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.64, MAG_FAINT_SEARCH_LIMIT=15.62)
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Considering the candidate 52818_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
Preparing report for the candidate 52818_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
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Considering the candidate 52847_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
The candidate 52847_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144 did not pass the final checks
**** FOUND 10:45:29.87 +03:06:09.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.72, MAG_FAINT_SEARCH_LIMIT=15.70)GAIADR2_OUTPUT=# 3.293 3809440214058269312 161.37512942221 +03.10326158751 14.7162 13.8497 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.293#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52854_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
The candidate 52854_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144 did not pass the final checks
**** FOUND 10:50:51.68 +01:40:03.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.82, MAG_FAINT_SEARCH_LIMIT=15.80)GAIADR2_OUTPUT=# 1.079 3808292255199867904 162.71562362015 +01.66761916606 14.8213 14.1675 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.079#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52857_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
The candidate 52857_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144 did not pass the final checks
**** FOUND 10:48:06.46 +03:11:31.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.96, MAG_FAINT_SEARCH_LIMIT=15.94)GAIADR2_OUTPUT=# 2.490 3809410905201449728 162.02715382112 +03.19146133854 14.7481 14.1026 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.490#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 03154_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144
The candidate 03154_fd_Leo-08-Q1b1x1_2026-04-13_23-56-50_20.00sec_-4.90C_LIGHTs_0144 did not pass the final checks