This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY
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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
W CrB,2461082.8444,11.18,0.05,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
W CrB 20260211.3444 11.18CV 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
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:15:24.60 +37:47:44.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20_00sec_-14_90C_LIGHT_0690_fits__*pix.png resample_wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20_00sec_-14_90C_LIGHT_0363_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20_00sec_-14_90C_LIGHT_0690_fits__*pix.png resample_wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20_00sec_-14_90C_LIGHT_0362_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20_00sec_-14_90C_LIGHT_0690_fits__*pix.png resample_wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20_00sec_-14_90C_LIGHT_0363_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20_00sec_-14_90C_LIGHT_0690_fits__*pix.png resample_wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20_00sec_-14_90C_LIGHT_0362_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 11.3444* 16 36 58.80 +42 44 50.1 10.1 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
MU Her,2461082.8444,10.12,0.05,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
MU Her 20260211.3444 10.12CV 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
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:36:58.80 +42:44:50.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20_00sec_-14_90C_LIGHT_0690_fits__*pix.png resample_wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20_00sec_-14_90C_LIGHT_0363_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20_00sec_-14_90C_LIGHT_0690_fits__*pix.png resample_wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20_00sec_-14_90C_LIGHT_0362_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20_00sec_-14_90C_LIGHT_0690_fits__*pix.png resample_wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20_00sec_-14_90C_LIGHT_0363_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20_00sec_-14_90C_LIGHT_0690_fits__*pix.png resample_wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20_00sec_-14_90C_LIGHT_0362_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461033.01864019 23.12.2025 12:26:40.512 /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits
First image: 2461033.01864019 23.12.2025 12:26:40.512 /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits
Last image: 2461082.84474983 11.02.2026 08:16:16.385 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.69
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): 7888
Objects passed selection criteria: 7883
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 7428.5
Average stars matched: 7324.5 (98.6 %)
Memory usage VmPeak: 113984 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Tue Feb 10 15:05:05 CST 2026
VaST build number 1.0rc88-299-g877bacc0
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Feb 11 02:19:38 CST 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: 2461033.01864019 23.12.2025 12:26:40.512 /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits
First image: 2461033.01864019 23.12.2025 12:26:40.512 /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits
Last image: 2461082.84474983 11.02.2026 08:16:16.385 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 49
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.41
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: 15 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): 47137
Objects passed selection criteria: 47043
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 45434.5
Average stars matched: 44142 (97.1552 %)
Memory usage VmPeak: 147372 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Tue Feb 10 15:05:05 CST 2026
VaST build number 1.0rc88-299-g877bacc0
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Feb 11 02:20:44 CST 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/CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits
SExtractor catalog cache: saved CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits.cat to cache
SExtractor catalog cache: saved CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.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/CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.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: 2461082.84400462
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'
Plate-solving the images
wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits exists and is non-empty
Saving wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits to local_wcs_cache/
'wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits' -> 'local_wcs_cache/wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits'
wcs_CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits exists and is non-empty
Saving wcs_CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits to local_wcs_cache/
'wcs_CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits' -> 'local_wcs_cache/wcs_CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits'
wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits exists and is non-empty
Saving wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits to local_wcs_cache/
'wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits' -> 'local_wcs_cache/wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits'
wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits exists and is non-empty
Saving wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits to local_wcs_cache/
'wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits' -> 'local_wcs_cache/wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.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 16:21:48.514 +38:00:43.10
Second-epoch image center 16:21:48.847 +38:00:05.11
Angular distance between the image centers 0.01 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 16:21:48.514 +38:00:43.10
Second-epoch image center 16:21:51.568 +38:00:34.12
Angular distance between the image centers 0.01 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 16:21:48.847 +38:00:05.11
Second-epoch second image center 16:21:51.568 +38:00:34.12
Angular distance between the image centers 0.01203 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/CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits &> /tmp/tmp.O1YWYA3uCt
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits &> /tmp/tmp.20NCIxK3RA
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits &> /tmp/tmp.TIobIdlJCb
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits &> /tmp/tmp.XbhyVCziDz
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits
Calibrating the magnitude scale
Found non-empty wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.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_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits and wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.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_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits and wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits.cat
Found non-empty wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits and wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits.cat
The reference image (wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits) and catalog (wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits.cat) found
'wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits.cat' -> 'wcsmag.cat'
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
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 5224 out of 8344 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.890718
a=0.000000 b=1.000000 c=22.890718
From vast_summary.log: estimated ref. image limiting mag.: -7.69
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.20
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.20
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits
2.1 pix CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits
2.1 pix fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits
2.1 pix fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits
Limiting magnitude estimates:
15.2 mag. CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits
15.2 mag. CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits
14.9 mag. fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits
14.9 mag. fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits
All-image limiting magnitude estimate: 14.9 (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 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.O1YWYA3uCt (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_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits' -> 'wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits
WCS_IMAGE_NAME=wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits
WCS-calibrated image found: wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits
Checking if the catalog wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits.cat corresponding to the image wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits alredy exist and is non-empty...
Catalog wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits.cat corresponding to the image wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits
WCS catalog name: wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=562, passed=8344
Got 8344 stars (including 7771 good ones) from the SExtractor catalog wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits.cat
util/solve_plate_with_UCAC5 got 8344 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (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...
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.27"
Estimated accuracy of the plate solution: 0.24"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits -region wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.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.20NCIxK3RA (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_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits' -> 'wcs_CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits
WCS_IMAGE_NAME=wcs_CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits
WCS-calibrated image found: wcs_CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits
Checking if the catalog wcs_CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits.cat corresponding to the image wcs_CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits alredy exist and is non-empty...
Catalog wcs_CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits.cat corresponding to the image wcs_CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits
WCS catalog name: wcs_CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=529, passed=8259
Got 8259 stars (including 7719 good ones) from the SExtractor catalog wcs_CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits.cat
util/solve_plate_with_UCAC5 got 8259 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (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...
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.28"
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits -region wcs_CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.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.TIobIdlJCb (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_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.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_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits
WCS_IMAGE_NAME=wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits
WCS-calibrated image found: wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits
Checking if the catalog wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits.cat corresponding to the image wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits alredy exist and is non-empty...
Catalog wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits.cat corresponding to the image wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits
WCS catalog name: wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=454, passed=6666
Got 6666 stars (including 6202 good ones) from the SExtractor catalog wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits.cat
util/solve_plate_with_UCAC5 got 6666 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.7'
Seting catalog search parameters based on the expected field of view 942.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013093 (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 0.010474 (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...
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
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...
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits -region wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.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.XbhyVCziDz (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_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.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_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits
WCS_IMAGE_NAME=wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits
WCS-calibrated image found: wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits
Checking if the catalog wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits.cat corresponding to the image wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits alredy exist and is non-empty...
Catalog wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits.cat corresponding to the image wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits
WCS catalog name: wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=456, passed=6655
Got 6655 stars (including 6192 good ones) from the SExtractor catalog wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits.cat
util/solve_plate_with_UCAC5 got 6655 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.7'
Seting catalog search parameters based on the expected field of view 942.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013093 (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 0.010474 (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...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
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...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits -region wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.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_fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits'
Saving fully-calibrated image wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits'
Preparing the HTML report for the field CrB-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20398.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out04046.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 4s
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 20398_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363
The candidate 20398_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363 did not pass the final checks
**** FOUND 16:27:57.24 +36:58:56.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 0.832 1331136194689123072 246.98869611271 +36.98244753483 12.0818 11.5205 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.832#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20402_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363
The candidate 20402_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363 did not pass the final checks
**** FOUND 16:29:07.88 +34:13:46.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04046_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363
Preparing report for the candidate 04046_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 5s
Prepared the HTML report for the field CrB-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 ####
16:15:24.60 +37:47:44.5
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/CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits
SExtractor catalog cache: saved CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits.cat to cache
SExtractor catalog cache: saved CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits
Creating symlink local_wcs_cache/wcs_CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits
Creating symlink local_wcs_cache/wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits
Creating symlink local_wcs_cache/wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.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_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits exists and is non-empty
wcs_CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits exists and is non-empty
wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits exists and is non-empty
wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.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 16:21:48.514 +38:00:43.10
Second-epoch image center 16:21:48.847 +38:00:05.11
Angular distance between the image centers 0.01 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 16:21:48.514 +38:00:43.10
Second-epoch image center 16:21:51.568 +38:00:34.12
Angular distance between the image centers 0.01 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 16:21:48.847 +38:00:05.11
Second-epoch second image center 16:21:51.568 +38:00:34.12
Angular distance between the image centers 0.01203 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/CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits &> /tmp/tmp.mpLKeA7mPn
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits &> /tmp/tmp.9M4SldSbEE
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits &> /tmp/tmp.Ilk1J6I0Ac
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits &> /tmp/tmp.d0r6kja5or
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits
Calibrating the magnitude scale
Found non-empty wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.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_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits and wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.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_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits and wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits.cat
Found non-empty wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits and wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits.cat
The reference image (wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits) and catalog (wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits.cat) found
'wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits.cat' -> 'wcsmag.cat'
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
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 5320 out of 49011 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.763814
a=0.000000 b=1.000000 c=22.763814
From vast_summary.log: estimated ref. image limiting mag.: -7.41
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.35
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.35
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 25 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits
2.0 pix CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits
1.9 pix fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits
2.0 pix fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits
Limiting magnitude estimates:
15.4 mag. CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits
15.3 mag. CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits
15.1 mag. fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits
15.1 mag. fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 14.5 (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 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.mpLKeA7mPn (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_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits' -> 'wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits
WCS_IMAGE_NAME=wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits
WCS-calibrated image found: wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits
Checking if the catalog wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits.cat corresponding to the image wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits alredy exist and is non-empty...
Catalog wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits.cat corresponding to the image wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits
WCS catalog name: wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits.cat
SExtractor catalog parsing summary: zero_flux=1, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=2439, passed=48999
Got 48999 stars (including 46492 good ones) from the SExtractor catalog wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits.cat
util/solve_plate_with_UCAC5 got 48999 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (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...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.29"
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits -region wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_CrB-01-Q1b1x1_2025-12-23_06-26-40_20.00sec_-14.90C_LIGHT_0690.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.9M4SldSbEE (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_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits' -> 'wcs_CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits
WCS_IMAGE_NAME=wcs_CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits
WCS-calibrated image found: wcs_CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits
Checking if the catalog wcs_CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits.cat corresponding to the image wcs_CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits alredy exist and is non-empty...
Catalog wcs_CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits.cat corresponding to the image wcs_CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits
WCS catalog name: wcs_CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=2367, passed=48952
Got 48952 stars (including 46502 good ones) from the SExtractor catalog wcs_CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits.cat
util/solve_plate_with_UCAC5 got 48952 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (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...
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.30"
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits -region wcs_CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_CrB-01-Q1b1x1_2025-12-23_06-27-36_20.00sec_-14.90C_LIGHT_0691.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.Ilk1J6I0Ac (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_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.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_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits
WCS_IMAGE_NAME=wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits
WCS-calibrated image found: wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits
Checking if the catalog wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits.cat corresponding to the image wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits alredy exist and is non-empty...
Catalog wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits.cat corresponding to the image wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits
WCS catalog name: wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=1680, passed=42559
Got 42559 stars (including 40800 good ones) from the SExtractor catalog wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits.cat
util/solve_plate_with_UCAC5 got 42559 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.7'
Seting catalog search parameters based on the expected field of view 942.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013093 (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 0.010474 (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...
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.38"
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 959 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits -region wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.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.d0r6kja5or (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_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.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_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits
WCS_IMAGE_NAME=wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits
WCS-calibrated image found: wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits
Checking if the catalog wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits.cat corresponding to the image wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits alredy exist and is non-empty...
Catalog wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits.cat corresponding to the image wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits
WCS catalog name: wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=1666, passed=42574
Got 42574 stars (including 40836 good ones) from the SExtractor catalog wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits.cat
util/solve_plate_with_UCAC5 got 42574 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.7'
Seting catalog search parameters based on the expected field of view 942.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013093 (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 0.010474 (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...
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.38"
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits -region wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.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_fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.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_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-15-11_20.00sec_-14.90C_LIGHT_0362.fits
Saving fully-calibrated image wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.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_2026-02-11_CI_CrB-01-Q1b1x1_021728_TTUQ1b1x1_10652_Bwft7iPY/wcs_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363.fits
Preparing the HTML report for the field CrB-01-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out53964.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53965.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53971.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53974.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53975.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53984.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53992.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54018.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54028.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54030.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54039.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54041.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54042.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54044.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54061.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54091.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out32547.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
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Considering the candidate 53964_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363
The candidate 53964_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363 did not pass the final checks
**** FOUND 16:18:24.66 +41:47:30.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)
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Considering the candidate 53965_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363
The candidate 53965_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363 did not pass the final checks
**** FOUND 16:49:00.57 +37:14:48.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)GAIADR2_OUTPUT=# 0.907 1351447644787423104 252.25267113960 +37.24675593299 14.3611 13.7960 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.907#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53971_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363
The candidate 53971_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363 did not pass the final checks
**** FOUND 16:35:14.57 +38:43:28.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 0.866 1331706257108001792 248.81100874676 +38.72449870561 13.9544 13.3109 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.866#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53972_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363
The candidate 53972_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363 did not pass the final checks
**** FOUND 16:15:28.79 +37:10:05.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53974_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363
The candidate 53974_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363 did not pass the final checks
**** FOUND 16:18:08.70 +32:51:29.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 0.170 1322561000424417792 244.53628979562 +32.85802233734 13.8488 13.2018 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.170#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53975_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363
The candidate 53975_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363 did not pass the final checks
**** FOUND 16:23:14.41 +42:57:59.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 0.783 1382202840441926144 245.81028506848 +42.96668038806 13.4932 12.8415 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.783#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53983_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363
The candidate 53983_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363 did not pass the final checks
**** FOUND 15:49:03.65 +32:46:50.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53984_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363
The candidate 53984_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363 did not pass the final checks
**** FOUND 16:55:43.77 +38:33:18.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.37, MAG_FAINT_SEARCH_LIMIT=12.35)GAIADR2_OUTPUT=# 1.570 1351954794525711232 253.93284388136 +38.55543047404 11.3296 10.8395 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.570#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53991_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363
The candidate 53991_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363 did not pass the final checks
**** FOUND 16:11:39.28 +36:24:08.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53992_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363
The candidate 53992_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363 did not pass the final checks
**** FOUND 16:37:10.16 +37:56:06.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 1.681 1331426603197465600 249.29208174490 +37.93564479578 12.7720 12.3865 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.681#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53993_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363
The candidate 53993_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363 did not pass the final checks
**** FOUND 16:11:36.98 +36:25:15.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53997_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363
The candidate 53997_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363 did not pass the final checks
**** FOUND 16:46:27.83 +38:24:06.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54008_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363
The candidate 54008_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363 did not pass the final checks
**** FOUND 16:19:02.79 +40:10:02.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54018_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363
The candidate 54018_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363 did not pass the final checks
**** FOUND 16:30:15.03 +35:55:41.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 2.203 1330817920432116736 247.56242384719 +35.92881209453 13.7550 13.2797 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.203#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54028_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363
The candidate 54028_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363 did not pass the final checks
**** FOUND 16:35:58.04 +36:31:38.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 3.582 1327965959068533504 248.99180352401 +36.52841147260 14.0894 13.6015 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.582#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54030_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363
The candidate 54030_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363 did not pass the final checks
**** FOUND 16:24:35.44 +34:57:53.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 1.812 1329183530757507968 246.14757202144 +34.96538633625 14.0201 13.4179 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.812#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54039_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363
The candidate 54039_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363 did not pass the final checks
**** FOUND 16:08:50.06 +35:34:06.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 4.217 1330046716104763904 242.20935183473 +35.56935166751 14.0614 13.3861 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.217#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54041_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363
The candidate 54041_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363 did not pass the final checks
**** FOUND 16:39:57.49 +37:32:05.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 2.931 1328444521504652288 249.98983319042 +37.53550288226 14.3354 13.7860 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.931#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54042_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363
The candidate 54042_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363 did not pass the final checks
**** FOUND 16:16:22.08 +42:27:59.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 2.842 1381945932678243968 244.09304871619 +42.46674050313 14.3613 13.9088 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.842#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54044_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363
The candidate 54044_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363 did not pass the final checks
**** FOUND 16:47:09.29 +36:02:30.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.11, MAG_FAINT_SEARCH_LIMIT=15.09)
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Considering the candidate 54061_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363
The candidate 54061_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363 did not pass the final checks
**** FOUND 16:54:51.94 +34:31:57.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 1.583 1314754502227486848 253.71638428388 +34.53296675083 14.4596 13.9579 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.583#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54091_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363
The candidate 54091_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363 did not pass the final checks
**** FOUND 16:27:51.36 +34:48:10.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.48, MAG_FAINT_SEARCH_LIMIT=15.46)GAIADR2_OUTPUT=# 0.359 1326257382423369600 246.96394332385 +34.80288405498 13.2257 10.9770 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.359#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 23948_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363
The candidate 23948_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363 did not pass the final checks
**** FOUND 16:15:24.59 +37:47:44.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 06634_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363
The candidate 06634_fd_CrB-01-Q1b1x1_2026-02-11_02-16-16_20.00sec_-14.90C_LIGHT_0363 did not pass the final checks