This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a
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 10.3547* 11 15 10.74 +01 22 53.3 12.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461140.8547,12.38,0.05,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 20260410.3547 12.38CV 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 10.3547* 11 04 36.29 +02 21 31.8 13.1 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,2461140.8547,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260410.3547 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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 10.3547* 10 41 35.15 +00 46 13.4 13.6 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,2461140.8547,13.58,0.05,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 20260410.3547 13.58CV 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!
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,2461140.8547,14.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260410.3547 14.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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 10.3547* 10 45 51.78 -04 45 34.2 14.3 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,2461140.8547,14.27,0.05,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 20260410.3547 14.27CV 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: 2461140.85509580 10.04.2026 08:31:10.277 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
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: 2 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 6283
Objects passed selection criteria: 6274
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 5543.5
Average stars matched: 5400.5 (97.4204 %)
Memory usage VmPeak: 112180 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Apr 10 06:23:08 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: 2461140.85509580 10.04.2026 08:31:10.277 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 50
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: 9 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 33324
Objects passed selection criteria: 33265
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: 31054.2
Average stars matched: 30160.2 (97.1212 %)
Memory usage VmPeak: 134716 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Apr 10 06:23:48 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_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.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_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.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: 2461140.85436237
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Leo-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_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits exists and is non-empty
Saving wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits to local_wcs_cache/
'wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits' -> 'local_wcs_cache/wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits'
wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.fits exists and is non-empty
Saving wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.fits to local_wcs_cache/
'wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.fits' -> 'local_wcs_cache/wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.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 11:08:30.196 -01:58:17.66
Angular distance between the image centers 0.0327 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 11:08:27.702 -01:58:53.86
Angular distance between the image centers 0.0337 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 11:08:30.196 -01:58:17.66
Second-epoch second image center 11:08:27.702 -01:58:53.86
Angular distance between the image centers 0.01446 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.zKsSFjP3az
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.OqO027OFWm
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_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits &> /tmp/tmp.MAmGxEXjat
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.fits &> /tmp/tmp.tyLibexNNG
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.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
2.3 pix fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits
2.3 pix fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.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
14.8 mag. fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits
14.8 mag. fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 11.8 (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.zKsSFjP3az (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_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/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.OqO027OFWm (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_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/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.MAmGxEXjat (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_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.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_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits
WCS_IMAGE_NAME=wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits
WCS-calibrated image found: wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits
Checking if the catalog wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits.cat corresponding to the image wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits.cat corresponding to the image wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.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_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits
WCS catalog name: wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=345, passed=4738
Got 4738 stars (including 4386 good ones) from the SExtractor catalog wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits.cat
util/solve_plate_with_UCAC5 got 4738 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 411 to 470 (Dec -7.7 to 3.8)
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: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 4693 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.8)
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(), 4694 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 4694 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
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_fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits -region wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.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.tyLibexNNG (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_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.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_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.fits
WCS_IMAGE_NAME=wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.fits
WCS-calibrated image found: wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.fits
Checking if the catalog wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.fits.cat corresponding to the image wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.fits.cat corresponding to the image wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.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_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.fits
WCS catalog name: wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=343, passed=4692
Got 4692 stars (including 4339 good ones) from the SExtractor catalog wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.fits.cat
util/solve_plate_with_UCAC5 got 4692 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 411 to 470 (Dec -7.7 to 3.8)
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(), 939 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 4649 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 411 to 470 (Dec -7.7 to 3.8)
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(), 4649 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 4649 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
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_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.fits -region wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.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_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/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_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/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_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits'
Saving fully-calibrated image wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.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: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20557_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
The candidate 20557_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203 did not pass the final checks
**** FOUND 10:46:17.26 +02:07:33.7 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 0s
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_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.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_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.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_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.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_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits exists and is non-empty
wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.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 11:08:30.196 -01:58:17.66
Angular distance between the image centers 0.0327 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 11:08:27.702 -01:58:53.86
Angular distance between the image centers 0.0337 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 11:08:30.196 -01:58:17.66
Second-epoch second image center 11:08:27.702 -01:58:53.86
Angular distance between the image centers 0.01446 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.jxHooRgJ8u
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.Y6xtou902q
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_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits &> /tmp/tmp.rwvh3fbqEw
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.fits &> /tmp/tmp.sByuvjl0Yh
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.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 50 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
2.0 pix fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits
2.0 pix fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.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
15.0 mag. fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits
15.0 mag. fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.fits
All-image limiting magnitude estimate: 15.0 (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.jxHooRgJ8u (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_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/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.Y6xtou902q (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_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/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.rwvh3fbqEw (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_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.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_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits
WCS_IMAGE_NAME=wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits
WCS-calibrated image found: wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits
Checking if the catalog wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits.cat corresponding to the image wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits.cat corresponding to the image wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.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_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits
WCS catalog name: wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=999, passed=28884
Got 28884 stars (including 27838 good ones) from the SExtractor catalog wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits.cat
util/solve_plate_with_UCAC5 got 28884 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 411 to 471 (Dec -7.7 to 3.8)
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(), 937 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 28635 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
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 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(), 28637 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 28638 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
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_fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits -region wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.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.sByuvjl0Yh (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_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.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_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.fits
WCS_IMAGE_NAME=wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.fits
WCS-calibrated image found: wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.fits
Checking if the catalog wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.fits.cat corresponding to the image wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.fits.cat corresponding to the image wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.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_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.fits
WCS catalog name: wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=984, passed=28881
Got 28881 stars (including 27851 good ones) from the SExtractor catalog wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.fits.cat
util/solve_plate_with_UCAC5 got 28881 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
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 411 to 470 (Dec -7.7 to 3.8)
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(), 940 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 28682 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
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 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(), 28682 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 28682 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
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_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.fits -region wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.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_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/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_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/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_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.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_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-30-06_20.00sec_-5.00C_LIGHTs_0202.fits
Saving fully-calibrated image wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.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_2026-04-10_CI_Leo-08-Q1b1x1_033205_TTUQ1b1x1_666_ndjcfq6a/wcs_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203.fits
Preparing the HTML report for the field Leo-08-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out51709.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52344.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52351.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52426.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52580.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52613.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52740.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52762.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52790.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52814.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52816.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52829.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52838.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52847.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52848.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52852.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out51952.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52096.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52264.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52529.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52591.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 51709_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
The candidate 51709_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203 did not pass the final checks
**** FOUND 11:01:05.17 -01:53:41.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.79, MAG_FAINT_SEARCH_LIMIT=15.77)GAIADR2_OUTPUT=# 0.739 3801880865459111040 165.27164925357 -01.89506372502 14.8498 14.1143 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.739#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51716_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
The candidate 51716_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203 did not pass the final checks
**** FOUND 11:02:26.12 +00:05:50.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51718_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
The candidate 51718_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203 did not pass the final checks
**** FOUND 11:32:30.21 +00:00:37.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51719_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
The candidate 51719_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203 did not pass the final checks
**** FOUND 11:25:44.97 +01:31:07.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51892_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
The candidate 51892_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203 did not pass the final checks
**** FOUND 11:06:45.00 +01:57:43.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51937_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
The candidate 51937_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203 did not pass the final checks
**** FOUND 10:46:17.24 +02:07:33.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51952_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
Preparing report for the candidate 51952_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
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Considering the candidate 52009_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
The candidate 52009_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203 did not pass the final checks
**** FOUND 11:34:19.07 -03:15:45.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52023_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
The candidate 52023_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203 did not pass the final checks
**** FOUND 10:53:27.79 +02:36:23.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52096_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
Preparing report for the candidate 52096_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
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Considering the candidate 52128_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
The candidate 52128_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203 did not pass the final checks
**** FOUND 11:20:24.08 -01:03:43.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52153_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
The candidate 52153_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203 did not pass the final checks
**** FOUND 11:29:07.33 -02:53:47.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52162_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
The candidate 52162_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203 did not pass the final checks
**** FOUND 11:24:33.38 +00:11:56.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52264_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
Preparing report for the candidate 52264_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
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Considering the candidate 52271_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
The candidate 52271_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203 did not pass the final checks
**** FOUND 10:50:44.34 -04:44:59.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52275_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
The candidate 52275_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203 did not pass the final checks
**** FOUND 11:14:03.15 +02:50:13.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52295_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
The candidate 52295_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203 did not pass the final checks
**** FOUND 10:41:13.22 -00:17:32.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52298_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
The candidate 52298_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203 did not pass the final checks
**** FOUND 11:05:57.95 -05:23:35.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52320_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
The candidate 52320_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203 did not pass the final checks
**** FOUND 11:05:54.92 +01:12:37.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52337_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
The candidate 52337_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203 did not pass the final checks
**** FOUND 10:46:55.90 -05:02:26.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52344_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
The candidate 52344_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203 did not pass the final checks
**** FOUND 10:37:41.30 -03:54:22.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 0.594 3778258339172642560 159.42221018318 -03.90635580974 13.5949 13.0892 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.594#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52351_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
The candidate 52351_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203 did not pass the final checks
**** FOUND 10:38:10.93 -04:11:18.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 3.436 3777863408339991552 159.54565357281 -04.18755212592 13.7846 13.2694 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.436#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52362_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
The candidate 52362_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203 did not pass the final checks
**** FOUND 10:52:36.17 -00:13:57.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 52409_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
The candidate 52409_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203 did not pass the final checks
**** FOUND 11:29:49.72 -04:58:11.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52422_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
The candidate 52422_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203 did not pass the final checks
**** FOUND 11:06:03.46 -07:01:30.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52426_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
The candidate 52426_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203 did not pass the final checks
**** FOUND 10:51:36.72 -02:35:51.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.05, MAG_FAINT_SEARCH_LIMIT=15.03)GAIADR2_OUTPUT=# 0.830 3801591552166674944 162.90308416205 -02.59796471367 13.9426 13.4703 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.830#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52440_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
The candidate 52440_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203 did not pass the final checks
**** FOUND 11:37:10.27 -00:48:33.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52529_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
Preparing report for the candidate 52529_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
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Considering the candidate 52538_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
The candidate 52538_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203 did not pass the final checks
**** FOUND 10:58:20.74 -02:03:39.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52554_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
The candidate 52554_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203 did not pass the final checks
**** FOUND 11:28:57.64 -06:48:35.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52575_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
The candidate 52575_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203 did not pass the final checks
**** FOUND 11:03:06.38 +01:32:24.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52580_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
The candidate 52580_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203 did not pass the final checks
**** FOUND 10:56:07.55 +00:24:33.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 2.907 3804820031839020544 164.03080482072 +00.40883138872 14.4620 13.9353 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.907#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52591_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
Preparing report for the candidate 52591_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
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Considering the candidate 52607_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
The candidate 52607_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203 did not pass the final checks
**** FOUND 11:39:49.02 +02:21:04.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52613_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
The candidate 52613_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203 did not pass the final checks
**** FOUND 10:55:22.98 +03:14:13.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 0.633 3809631460361944832 163.84592572635 +03.23701462513 14.2591 13.6714 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.633#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52668_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
The candidate 52668_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203 did not pass the final checks
**** FOUND 11:31:18.92 -06:36:04.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52671_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
The candidate 52671_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203 did not pass the final checks
**** FOUND 11:18:46.59 -06:17:09.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52730_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
The candidate 52730_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203 did not pass the final checks
**** FOUND 11:27:31.73 -03:42:37.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52740_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
The candidate 52740_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203 did not pass the final checks
**** FOUND 11:23:31.16 -06:36:40.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.56, MAG_FAINT_SEARCH_LIMIT=15.54)GAIADR2_OUTPUT=# 2.881 3783867802684269056 170.88052985183 -06.61159642649 14.7201 14.2028 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.881#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52762_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
The candidate 52762_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203 did not pass the final checks
**** FOUND 11:15:44.06 +02:54:26.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.62, MAG_FAINT_SEARCH_LIMIT=15.60)GAIADR2_OUTPUT=# 2.811 3811787808822811264 168.93422498041 +02.90685963935 15.1730 14.8288 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.811#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52787_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
The candidate 52787_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203 did not pass the final checks
**** FOUND 11:16:40.43 +02:49:07.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52790_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
The candidate 52790_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203 did not pass the final checks
**** FOUND 11:27:33.58 +00:05:49.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.64, MAG_FAINT_SEARCH_LIMIT=15.62)GAIADR2_OUTPUT=# 2.954 3797477596267921280 171.89057460171 +00.09757367635 14.9011 14.3516 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.954#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52814_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
The candidate 52814_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203 did not pass the final checks
**** FOUND 11:32:11.25 -05:32:26.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.57, MAG_FAINT_SEARCH_LIMIT=15.55)GAIADR2_OUTPUT=# 1.219 3785867509393014784 173.04719133794 -05.54068000884 14.7133 14.1777 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.219#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52816_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
The candidate 52816_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203 did not pass the final checks
**** FOUND 11:04:57.63 -02:00:14.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.74, MAG_FAINT_SEARCH_LIMIT=15.72)GAIADR2_OUTPUT=# 2.584 3803326585810780160 166.24078475005 -02.00360492470 14.9934 14.2038 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.584#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52829_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
The candidate 52829_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203 did not pass the final checks
**** FOUND 10:51:52.94 +02:41:48.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.91, MAG_FAINT_SEARCH_LIMIT=15.89)GAIADR2_OUTPUT=# 3.434 3809503607775850752 162.97132710069 +02.69623507113 14.4504 13.3321 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.434#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52838_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
The candidate 52838_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203 did not pass the final checks
**** FOUND 11:08:01.97 +02:01:20.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.71, MAG_FAINT_SEARCH_LIMIT=15.69)GAIADR2_OUTPUT=# 1.263 3811275470763970816 167.00796537948 +02.02255893964 14.8492 14.2469 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.263#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52840_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
The candidate 52840_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203 did not pass the final checks
**** FOUND 11:28:30.25 -02:51:05.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52847_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
The candidate 52847_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203 did not pass the final checks
**** FOUND 11:23:22.69 +02:41:10.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.95, MAG_FAINT_SEARCH_LIMIT=15.93)GAIADR2_OUTPUT=# 1.326 3810875042373178880 170.84453144779 +02.68577082527 14.9916 14.3417 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.326#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52848_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
The candidate 52848_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203 did not pass the final checks
**** FOUND 10:52:55.15 -05:49:24.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.88, MAG_FAINT_SEARCH_LIMIT=15.86)GAIADR2_OUTPUT=# 0.117 3764871682025356416 163.22980420020 -05.82350225342 14.6382 13.7051 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.117#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52852_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203
The candidate 52852_fd_Leo-08-Q1b1x1_2026-04-10_03-31-10_20.00sec_-4.90C_LIGHTs_0203 did not pass the final checks