This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA
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!
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,2461139.7751,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260409.2751 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461139.7751,12.63,0.05,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 20260409.2751 12.63CV 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,2461139.7751,13.16,0.05,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 20260409.2751 13.16CV 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,2461139.7751,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260409.2751 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461082.92034660 11.02.2026 10:05:07.946 /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
First image: 2461082.92034660 11.02.2026 10:05:07.946 /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
Last image: 2461139.77539521 09.04.2026 06:36:24.146 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 13
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.93
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 6707
Objects passed selection criteria: 6697
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: 6189.25
Average stars matched: 5823.5 (94.0906 %)
Memory usage VmPeak: 112244 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 Thu Apr 9 01:38:17 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: 2461082.92034660 11.02.2026 10:05:07.946 /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
First image: 2461082.92034660 11.02.2026 10:05:07.946 /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
Last image: 2461139.77539521 09.04.2026 06:36:24.146 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 29
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.63
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: 11 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): 37485
Objects passed selection criteria: 37395
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 34553.8
Average stars matched: 33402 (96.6668 %)
Memory usage VmPeak: 138552 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 Thu Apr 9 01:39:05 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/Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits
SExtractor catalog cache: saved Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits.cat to cache
SExtractor catalog cache: saved Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.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/Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.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: 2461139.77472021
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_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits exists and is non-empty
Saving wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits to local_wcs_cache/
'wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits' -> 'local_wcs_cache/wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits'
wcs_Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits exists and is non-empty
Saving wcs_Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits to local_wcs_cache/
'wcs_Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits' -> 'local_wcs_cache/wcs_Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits'
wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits exists and is non-empty
Saving wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits to local_wcs_cache/
'wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits' -> 'local_wcs_cache/wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits'
wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits exists and is non-empty
Saving wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits to local_wcs_cache/
'wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits' -> 'local_wcs_cache/wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.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 12:26:39.749 -18:00:06.86
Second-epoch image center 12:26:49.740 -17:57:53.50
Angular distance between the image centers 0.0542 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 12:26:39.749 -18:00:06.86
Second-epoch image center 12:26:51.742 -17:58:30.87
Angular distance between the image centers 0.0545 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 12:26:49.740 -17:57:53.50
Second-epoch second image center 12:26:51.742 -17:58:30.87
Angular distance between the image centers 0.01307 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/Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits &> /tmp/tmp.0DwygXgFCe
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits &> /tmp/tmp.66Ny8yu7wZ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits &> /tmp/tmp.7pDAVpEDTm
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits &> /tmp/tmp.Ux966qFCcW
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits
Calibrating the magnitude scale
Found non-empty wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.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_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits and wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.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_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits and wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits.cat
Found non-empty wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits and wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits.cat
The reference image (wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits) and catalog (wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits.cat) found
'wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits.cat' -> 'wcsmag.cat'
Read 5826 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 178.3232 to 195.2856 deg, Dec -23.3230 to -12.5315 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 178.3232 to 195.2856 deg, Dec -23.3230 to -12.5315 deg
Loaded 5194 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): 3909 out of 4081 total matches.
Matched with Tycho-2 4081 out of 5826 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.822012
a=0.000000 b=1.000000 c=22.822012
From vast_summary.log: estimated ref. image limiting mag.: -7.93
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.89
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.89
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 13 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
2.1 pix Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
3.6 pix fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits
3.5 pix fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits
Limiting magnitude estimates:
14.9 mag. Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
14.9 mag. Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
14.7 mag. fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits
14.7 mag. fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 11.9 (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.0DwygXgFCe (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_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits' -> 'wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
WCS_IMAGE_NAME=wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
WCS-calibrated image found: wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
Checking if the catalog wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits.cat corresponding to the image wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits alredy exist and is non-empty...
Catalog wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits.cat corresponding to the image wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
WCS catalog name: wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=465, passed=5826
Got 5826 stars (including 5355 good ones) from the SExtractor catalog wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits.cat
util/solve_plate_with_UCAC5 got 5826 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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 5723 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 5724 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 5724 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits -region wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.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.66Ny8yu7wZ (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_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits' -> 'wcs_Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
WCS_IMAGE_NAME=wcs_Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
WCS-calibrated image found: wcs_Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
Checking if the catalog wcs_Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits.cat corresponding to the image wcs_Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits alredy exist and is non-empty...
Catalog wcs_Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits.cat corresponding to the image wcs_Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
WCS catalog name: wcs_Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=457, passed=5792
Got 5792 stars (including 5328 good ones) from the SExtractor catalog wcs_Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits.cat
util/solve_plate_with_UCAC5 got 5792 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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 967 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 5668 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 5668 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 5668 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 979 stars left (next iteration limit 1076)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits -region wcs_Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.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.7pDAVpEDTm (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_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.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_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits
WCS_IMAGE_NAME=wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits
WCS-calibrated image found: wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits
Checking if the catalog wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits.cat corresponding to the image wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits alredy exist and is non-empty...
Catalog wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits.cat corresponding to the image wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits
WCS catalog name: wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=308, passed=6637
Got 6637 stars (including 6324 good ones) from the SExtractor catalog wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits.cat
util/solve_plate_with_UCAC5 got 6637 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 332 to 391 (Dec -23.5 to -12.1)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 968 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 6552 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 332 to 391 (Dec -23.5 to -12.1)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 6551 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 6551 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 978 stars left (next iteration limit 1075)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits -region wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.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.Ux966qFCcW (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_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.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_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits
WCS_IMAGE_NAME=wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits
WCS-calibrated image found: wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits
Checking if the catalog wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits.cat corresponding to the image wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits alredy exist and is non-empty...
Catalog wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits.cat corresponding to the image wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits
WCS catalog name: wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=326, passed=6668
Got 6668 stars (including 6337 good ones) from the SExtractor catalog wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits.cat
util/solve_plate_with_UCAC5 got 6668 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 332 to 391 (Dec -23.6 to -12.1)
Done reading UCAC5 zone files...
Matched 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 970 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 6590 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 332 to 391 (Dec -23.6 to -12.1)
Done reading UCAC5 zone files...
Matched 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 6589 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 980 matched stars entering correct_measured_positions(), 6589 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 980 stars left (next iteration limit 1078)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits -region wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.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_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits'
Saving fully-calibrated image wcs_Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/wcs_Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits'
Saving fully-calibrated image wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits'
Saving fully-calibrated image wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits'
Preparing the HTML report for the field Crv-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20262.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20263.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20425.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20445.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20262_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168
The candidate 20262_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168 did not pass the final checks
**** FOUND 12:20:55.64 -21:09:56.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.89, MAG_FAINT_SEARCH_LIMIT=12.87)GAIADR2_OUTPUT=# 1.489 3514601017109794432 185.23220872716 -21.16558535928 11.9883 11.5112 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.489#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20263_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168
The candidate 20263_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168 did not pass the final checks
**** FOUND 12:47:48.79 -14:02:42.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.24, MAG_FAINT_SEARCH_LIMIT=12.22)GAIADR2_OUTPUT=# 0.309 3525608090576374912 191.95336769582 -14.04509929619 11.0790 10.4037 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.309#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20328_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168
The candidate 20328_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168 did not pass the final checks
**** FOUND 12:19:37.95 -19:15:21.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20425_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168
The candidate 20425_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168 did not pass the final checks
**** FOUND 12:34:00.68 -17:50:53.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.80, MAG_FAINT_SEARCH_LIMIT=12.78)GAIADR2_OUTPUT=# 0.630 3517185797148131200 188.50265245569 -17.84819837243 10.8294 9.5430 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.630#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20426_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168
The candidate 20426_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168 did not pass the final checks
**** FOUND 12:32:29.25 -18:43:53.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20428_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168
The candidate 20428_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168 did not pass the final checks
**** FOUND 12:46:09.16 -14:49:07.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20431_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168
The candidate 20431_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168 did not pass the final checks
**** FOUND 12:53:50.75 -13:50:45.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20434_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168
The candidate 20434_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168 did not pass the final checks
**** FOUND 12:20:05.72 -14:08:03.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20443_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168
The candidate 20443_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168 did not pass the final checks
**** FOUND 12:27:24.60 -18:22:20.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20445_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168
The candidate 20445_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168 did not pass the final checks
**** FOUND 12:26:15.80 -18:36:17.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.95, MAG_FAINT_SEARCH_LIMIT=12.93)GAIADR2_OUTPUT=# 0.413 3519713398286430720 186.56592380930 -18.60486808268 11.7968 11.2724 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.413#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20447_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168
The candidate 20447_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168 did not pass the final checks
**** FOUND 12:20:32.38 -16:22:38.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20456_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168
The candidate 20456_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168 did not pass the final checks
**** FOUND 12:21:52.49 -13:53:10.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02998_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168
The candidate 02998_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168 did not pass the final checks
**** FOUND 12:35:02.05 -18:27:39.4 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Crv-01-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/Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits
SExtractor catalog cache: saved Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits.cat to cache
SExtractor catalog cache: saved Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
Creating symlink local_wcs_cache/wcs_Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
Creating symlink local_wcs_cache/wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits
Creating symlink local_wcs_cache/wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.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_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits exists and is non-empty
wcs_Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits exists and is non-empty
wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits exists and is non-empty
wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.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 12:26:39.749 -18:00:06.86
Second-epoch image center 12:26:49.740 -17:57:53.50
Angular distance between the image centers 0.0542 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 12:26:39.749 -18:00:06.86
Second-epoch image center 12:26:51.742 -17:58:30.87
Angular distance between the image centers 0.0545 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 12:26:49.740 -17:57:53.50
Second-epoch second image center 12:26:51.742 -17:58:30.87
Angular distance between the image centers 0.01307 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/Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits &> /tmp/tmp.AwCwvBg0S0
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits &> /tmp/tmp.yLR0FVJ28w
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits &> /tmp/tmp.JEmv56D8FQ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits &> /tmp/tmp.kQ71R2hNly
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits
Calibrating the magnitude scale
Found non-empty wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.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_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits and wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.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_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits and wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits.cat
Found non-empty wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits and wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits.cat
The reference image (wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits) and catalog (wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits.cat) found
'wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits.cat' -> 'wcsmag.cat'
Read 38658 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 178.2863 to 195.3102 deg, Dec -23.3302 to -12.4639 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 178.2863 to 195.3102 deg, Dec -23.3302 to -12.4639 deg
Loaded 5234 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): 4057 out of 4444 total matches.
Matched with Tycho-2 4444 out of 38658 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.659516
a=0.000000 b=1.000000 c=22.659516
From vast_summary.log: estimated ref. image limiting mag.: -7.63
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.03
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.03
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 29 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
1.9 pix Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
3.2 pix fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits
3.2 pix fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits
Limiting magnitude estimates:
15.0 mag. Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
15.0 mag. Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
14.7 mag. fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits
14.8 mag. fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 14.1 (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.AwCwvBg0S0 (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_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits' -> 'wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
WCS_IMAGE_NAME=wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
WCS-calibrated image found: wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
Checking if the catalog wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits.cat corresponding to the image wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits alredy exist and is non-empty...
Catalog wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits.cat corresponding to the image wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
WCS catalog name: wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=1533, passed=38642
Got 38642 stars (including 37036 good ones) from the SExtractor catalog wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits.cat
util/solve_plate_with_UCAC5 got 38642 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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 971 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 38118 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 38118 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 38118 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 978 stars left (next iteration limit 1075)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits -region wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.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.yLR0FVJ28w (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_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits' -> 'wcs_Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
WCS_IMAGE_NAME=wcs_Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
WCS-calibrated image found: wcs_Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
Checking if the catalog wcs_Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits.cat corresponding to the image wcs_Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits alredy exist and is non-empty...
Catalog wcs_Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits.cat corresponding to the image wcs_Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
WCS catalog name: wcs_Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=1495, passed=38320
Got 38320 stars (including 36755 good ones) from the SExtractor catalog wcs_Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits.cat
util/solve_plate_with_UCAC5 got 38320 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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 966 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 37640 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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 37640 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 37640 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 978 stars left (next iteration limit 1075)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits -region wcs_Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.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.JEmv56D8FQ (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_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.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_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits
WCS_IMAGE_NAME=wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits
WCS-calibrated image found: wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits
Checking if the catalog wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits.cat corresponding to the image wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits alredy exist and is non-empty...
Catalog wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits.cat corresponding to the image wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits
WCS catalog name: wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=1059, passed=30670
Got 30670 stars (including 29582 good ones) from the SExtractor catalog wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits.cat
util/solve_plate_with_UCAC5 got 30670 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 332 to 391 (Dec -23.5 to -12.1)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 30310 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 332 to 391 (Dec -23.5 to -12.1)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 30310 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 30310 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 978 stars left (next iteration limit 1075)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits -region wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.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.kQ71R2hNly (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_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.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_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits
WCS_IMAGE_NAME=wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits
WCS-calibrated image found: wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits
Checking if the catalog wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits.cat corresponding to the image wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits alredy exist and is non-empty...
Catalog wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits.cat corresponding to the image wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits
WCS catalog name: wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=1063, passed=31465
Got 31465 stars (including 30374 good ones) from the SExtractor catalog wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits.cat
util/solve_plate_with_UCAC5 got 31465 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 332 to 391 (Dec -23.6 to -12.1)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 968 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 31097 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
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 332 to 391 (Dec -23.6 to -12.1)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 31099 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 31099 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 979 stars left (next iteration limit 1076)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits -region wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.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_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.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_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/wcs_Crv-01-Q1b1x1_2026-02-11_04-05-07_20.00sec_-14.90C_LIGHT_0477.fits
Saving fully-calibrated image wcs_Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.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_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/wcs_Crv-01-Q1b1x1_2026-02-11_04-05-59_20.00sec_-15.00C_LIGHT_0478.fits
Saving fully-calibrated image wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.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_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-35-25_20.00sec_-4.90C_LIGHTs_0167.fits
Saving fully-calibrated image wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.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_2026-04-09_CI_Crv-01-Q1b1x1_013727_TTUQ1b1x1_10832_cutgjieA/wcs_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168.fits
Preparing the HTML report for the field Crv-01-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out52793.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52931.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53111.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53854.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53896.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53899.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53907.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53915.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53924.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53931.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53971.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53975.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out53019.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53130.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53259.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53282.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52793_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168
The candidate 52793_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168 did not pass the final checks
**** FOUND 12:21:00.94 -13:06:49.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.97, MAG_FAINT_SEARCH_LIMIT=14.95)GAIADR2_OUTPUT=# 3.368 3576203286359927040 185.25487693877 -13.11364533553 14.1499 12.9213 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.368#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52931_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168
The candidate 52931_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168 did not pass the final checks
**** FOUND 12:34:00.02 -14:37:58.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.68, MAG_FAINT_SEARCH_LIMIT=12.66)GAIADR2_OUTPUT=# 1.352 3526876171080795648 188.50046651521 -14.63277389081 11.7629 11.2470 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.352#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53019_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168
Preparing report for the candidate 53019_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53091_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168
The candidate 53091_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168 did not pass the final checks
**** FOUND 12:40:32.30 -17:38:51.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53111_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168
The candidate 53111_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168 did not pass the final checks
**** FOUND 12:01:06.67 -17:25:00.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 2.762 3567340020049534080 180.27698844502 -17.41679986708 11.8895 10.1871 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.762#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53130_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168
Preparing report for the candidate 53130_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53152_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168
The candidate 53152_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168 did not pass the final checks
**** FOUND 12:32:47.54 -16:41:14.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53259_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168
Preparing report for the candidate 53259_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53282_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168
Preparing report for the candidate 53282_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53416_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168
The candidate 53416_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168 did not pass the final checks
**** FOUND 12:13:01.52 -17:08:44.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53601_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168
The candidate 53601_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168 did not pass the final checks
**** FOUND 12:03:14.85 -14:46:11.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53849_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168
The candidate 53849_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168 did not pass the final checks
**** FOUND 11:56:45.68 -13:00:19.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53854_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168
The candidate 53854_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168 did not pass the final checks
**** FOUND 12:59:01.95 -15:15:26.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 0.611 3524341556260610816 194.75812812717 -15.25744734527 14.0018 13.1732 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.611#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53861_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168
The candidate 53861_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168 did not pass the final checks
**** FOUND 12:14:48.50 -17:38:44.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53896_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168
The candidate 53896_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168 did not pass the final checks
**** FOUND 12:05:35.57 -15:15:21.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)GAIADR2_OUTPUT=# 1.249 3570257161836576000 181.39834413103 -15.25634901609 14.1505 13.1190 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.249#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53899_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168
The candidate 53899_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168 did not pass the final checks
**** FOUND 12:04:15.18 -15:16:51.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.32, MAG_FAINT_SEARCH_LIMIT=15.30)GAIADR2_OUTPUT=# 3.052 3570300833063999488 181.06400163459 -15.28149504527 14.4706 13.9219 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.052#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53907_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168
The candidate 53907_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168 did not pass the final checks
**** FOUND 12:58:16.36 -13:22:23.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.35, MAG_FAINT_SEARCH_LIMIT=15.33)GAIADR2_OUTPUT=# 1.220 3525975739777055616 194.56824377192 -13.37346939184 14.3611 13.8107 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.220#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53915_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168
The candidate 53915_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168 did not pass the final checks
**** FOUND 12:09:32.10 -12:55:59.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.62, MAG_FAINT_SEARCH_LIMIT=15.60)GAIADR2_OUTPUT=# 0.986 3571190475409843072 182.38356322666 -12.93337131500 14.5794 14.0803 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.986#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53924_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168
The candidate 53924_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168 did not pass the final checks
**** FOUND 12:52:10.14 -13:29:15.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.35, MAG_FAINT_SEARCH_LIMIT=15.33)GAIADR2_OUTPUT=# 1.437 3526108059129684352 193.04200875529 -13.48793400740 14.3961 13.7993 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.437#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53931_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168
The candidate 53931_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168 did not pass the final checks
**** FOUND 12:13:32.34 -14:19:18.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.53, MAG_FAINT_SEARCH_LIMIT=15.51)GAIADR2_OUTPUT=# 0.802 3570058596908394112 183.38481571432 -14.32170328984 14.5985 14.0422 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.802#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53948_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168
The candidate 53948_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168 did not pass the final checks
**** FOUND 11:55:38.20 -17:05:51.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53956_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168
The candidate 53956_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168 did not pass the final checks
**** FOUND 12:06:19.85 -17:20:08.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53964_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168
The candidate 53964_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168 did not pass the final checks
**** FOUND 12:53:21.84 -13:26:31.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53971_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168
The candidate 53971_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168 did not pass the final checks
**** FOUND 12:44:20.24 -13:10:29.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.71, MAG_FAINT_SEARCH_LIMIT=15.69)GAIADR2_OUTPUT=# 0.850 3528903258205499776 191.08419162426 -13.17491369731 14.6894 14.1829 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.850#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53975_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168
The candidate 53975_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168 did not pass the final checks
**** FOUND 12:31:08.89 -13:00:55.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.62, MAG_FAINT_SEARCH_LIMIT=15.60)GAIADR2_OUTPUT=# 0.704 3528401743464623488 187.78719903871 -13.01518410491 14.6573 13.8610 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.704#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54003_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168
The candidate 54003_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168 did not pass the final checks
**** FOUND 12:03:28.12 -17:49:53.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20083_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168
The candidate 20083_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168 did not pass the final checks
**** FOUND 12:35:02.04 -18:27:39.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28390_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168
The candidate 28390_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168 did not pass the final checks
**** FOUND 12:19:37.94 -19:15:22.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03548_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168
The candidate 03548_fd_Crv-01-Q1b1x1_2026-04-09_01-36-24_20.00sec_-4.90C_LIGHTs_0168 did not pass the final checks