This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 25.2602* 10 42 50.64 +00 24 40.3 11.5 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461124.7602,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260325.2602 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:42:50.64 +00:24:40.3 ;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_Sex-02-Q2b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20_00sec_-14_90C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20_00sec_-15_00C_LIGHT_0038_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20_00sec_-15_00C_LIGHT_0038_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 03 25.2602* 10 14 36.75 +01 28 41.8 13.2 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461124.7602,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260325.2602 13.22CV 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/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:14:36.75 +01:28:41.8 ;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_Sex-02-Q2b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20_00sec_-14_90C_LIGHT_0039_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20_00sec_-15_00C_LIGHT_0038_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20_00sec_-14_90C_LIGHT_0039_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20_00sec_-14_90C_LIGHT_0453_fits__*pix.png resample_wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20_00sec_-15_00C_LIGHT_0038_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: 2461058.90489140 18.01.2026 09:42:52.617 /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
First image: 2461058.90489140 18.01.2026 09:42:52.617 /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
Last image: 2461124.76049851 25.03.2026 06:14:57.071 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.70
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 2 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 6141
Objects passed selection criteria: 6125
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 5160.75
Average stars matched: 5067 (98.1834 %)
Memory usage VmPeak: 112856 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Mar 25 01:22:05 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.90489140 18.01.2026 09:42:52.617 /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
First image: 2461058.90489140 18.01.2026 09:42:52.617 /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
Last image: 2461124.76049851 25.03.2026 06:14:57.071 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 45
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.42
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 9 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 32739
Objects passed selection criteria: 32681
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 29566
Average stars matched: 28896 (97.7339 %)
Memory usage VmPeak: 137424 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Mar 25 01:22:48 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_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 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits
SExtractor catalog cache: saved Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat to cache
SExtractor catalog cache: saved Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.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/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.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: 2461124.75987880
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_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits exists and is non-empty
Saving wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits to local_wcs_cache/
'wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits' -> 'local_wcs_cache/wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits'
wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits exists and is non-empty
Saving wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits to local_wcs_cache/
'wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits' -> 'local_wcs_cache/wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits'
wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits exists and is non-empty
Saving wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits to local_wcs_cache/
'wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits' -> 'local_wcs_cache/wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits'
wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits exists and is non-empty
Saving wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits to local_wcs_cache/
'wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits' -> 'local_wcs_cache/wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.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 10:17:03.829 -01:59:47.05
Second-epoch image center 10:17:10.229 -02:00:03.79
Angular distance between the image centers 0.03 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 10:17:03.829 -01:59:47.05
Second-epoch image center 10:17:07.390 -01:59:41.18
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 10:17:10.229 -02:00:03.79
Second-epoch second image center 10:17:07.390 -01:59:41.18
Angular distance between the image centers 0.01339 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/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits &> /tmp/tmp.Gr5ODpqeTW
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits &> /tmp/tmp.LeZk1a2o3q
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits &> /tmp/tmp.JUbPKqAuaG
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits &> /tmp/tmp.QQMKUHD5va
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits
Calibrating the magnitude scale
Found non-empty wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.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_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits and wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.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_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits and wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat
Found non-empty wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits and wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat
The reference image (wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits) and catalog (wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat) found
'wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.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 4187 out of 7808 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.873667
a=0.000000 b=1.000000 c=22.873667
From vast_summary.log: estimated ref. image limiting mag.: -7.70
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.17
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.17
Magnitude calibration plot:
____ 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:
2.3 pix Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
2.3 pix Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
2.3 pix fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits
2.3 pix fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits
Limiting magnitude estimates:
15.2 mag. Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
15.2 mag. Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
14.5 mag. fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits
14.5 mag. fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 11.6 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.Gr5ODpqeTW (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits is already a symlink and we do not allow symlinks on symlinks
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_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits' -> 'wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
WCS_IMAGE_NAME=wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
WCS-calibrated image found: wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
Checking if the catalog wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat corresponding to the image wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits alredy exist and is non-empty...
Catalog wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat corresponding to the image wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
WCS catalog name: wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=466, passed=7808
Got 7808 stars (including 7337 good ones) from the SExtractor catalog wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat
util/solve_plate_with_UCAC5 got 7808 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 931 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 931 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: 0.28"
Excluding outliers - 931 stars left (next iteration limit 1024)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits -region wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.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.LeZk1a2o3q (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits is already a symlink and we do not allow symlinks on symlinks
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_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits' -> 'wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
WCS_IMAGE_NAME=wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
WCS-calibrated image found: wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
Checking if the catalog wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat corresponding to the image wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits alredy exist and is non-empty...
Catalog wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat corresponding to the image wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
WCS catalog name: wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=461, passed=7862
Got 7862 stars (including 7394 good ones) from the SExtractor catalog wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat
util/solve_plate_with_UCAC5 got 7862 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 934 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 934 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 - 934 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits -region wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.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.JUbPKqAuaG (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_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.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_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits
WCS_IMAGE_NAME=wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits
WCS-calibrated image found: wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits
Checking if the catalog wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits.cat corresponding to the image wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits alredy exist and is non-empty...
Catalog wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits.cat corresponding to the image wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits
WCS catalog name: wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=268, passed=4797
Got 4797 stars (including 4525 good ones) from the SExtractor catalog wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits.cat
util/solve_plate_with_UCAC5 got 4797 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 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 930 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: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
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 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.46"
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 930 stars left (next iteration limit 1023)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits -region wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.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.QQMKUHD5va (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_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.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_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits
WCS_IMAGE_NAME=wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits
WCS-calibrated image found: wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits
Checking if the catalog wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits.cat corresponding to the image wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits alredy exist and is non-empty...
Catalog wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits.cat corresponding to the image wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits
WCS catalog name: wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=256, passed=4771
Got 4771 stars (including 4507 good ones) from the SExtractor catalog wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits.cat
util/solve_plate_with_UCAC5 got 4771 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 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 928 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: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
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 928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.43"
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 928 stars left (next iteration limit 1020)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits -region wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.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_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits'
Saving fully-calibrated image wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits'
Saving fully-calibrated image wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits'
Saving fully-calibrated image wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits'
Preparing the HTML report for the field Sex-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out20358.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20351_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039
The candidate 20351_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039 did not pass the final checks
**** FOUND 09:57:22.40 -02:32:55.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20358_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039
Preparing report for the candidate 20358_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02522_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039
The candidate 02522_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039 did not pass the final checks
**** FOUND 10:34:55.96 -00:20:33.9 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 7s
Prepared the HTML report for the field Sex-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
10:42:50.64 +00:24:40.3
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 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits
SExtractor catalog cache: saved Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat to cache
SExtractor catalog cache: saved Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
Creating symlink local_wcs_cache/wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
Creating symlink local_wcs_cache/wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits
Creating symlink local_wcs_cache/wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.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_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits exists and is non-empty
wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits exists and is non-empty
wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits exists and is non-empty
wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.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 10:17:03.829 -01:59:47.05
Second-epoch image center 10:17:10.229 -02:00:03.79
Angular distance between the image centers 0.03 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 10:17:03.829 -01:59:47.05
Second-epoch image center 10:17:07.390 -01:59:41.18
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 10:17:10.229 -02:00:03.79
Second-epoch second image center 10:17:07.390 -01:59:41.18
Angular distance between the image centers 0.01339 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/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits &> /tmp/tmp.oDtZNGW4Lg
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits &> /tmp/tmp.sMWInYZaLt
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits &> /tmp/tmp.ads0c5eYRE
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits &> /tmp/tmp.xpy1YEDVDN
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits
Calibrating the magnitude scale
Found non-empty wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.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_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits and wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.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_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits and wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat
Found non-empty wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits and wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat
The reference image (wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits) and catalog (wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat) found
'wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.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 4239 out of 40923 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.755743
a=0.000000 b=1.000000 c=22.755743
From vast_summary.log: estimated ref. image limiting mag.: -7.42
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.34
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.34
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 33 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
2.3 pix Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
2.2 pix fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits
2.2 pix fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits
Limiting magnitude estimates:
15.3 mag. Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
15.3 mag. Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
14.7 mag. fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits
14.7 mag. fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 14.1 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.oDtZNGW4Lg (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits is already a symlink and we do not allow symlinks on symlinks
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_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits' -> 'wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
WCS_IMAGE_NAME=wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
WCS-calibrated image found: wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
Checking if the catalog wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat corresponding to the image wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits alredy exist and is non-empty...
Catalog wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat corresponding to the image wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
WCS catalog name: wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=1914, passed=40911
Got 40911 stars (including 38933 good ones) from the SExtractor catalog wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat
util/solve_plate_with_UCAC5 got 40911 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 929 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: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.31"
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 929 stars left (next iteration limit 1021)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits -region wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.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.sMWInYZaLt (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits is already a symlink and we do not allow symlinks on symlinks
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_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits' -> 'wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
WCS_IMAGE_NAME=wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
WCS-calibrated image found: wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
Checking if the catalog wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat corresponding to the image wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits alredy exist and is non-empty...
Catalog wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat corresponding to the image wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
WCS catalog name: wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=1902, passed=40634
Got 40634 stars (including 38663 good ones) from the SExtractor catalog wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat
util/solve_plate_with_UCAC5 got 40634 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 931 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: 0.30"
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 931 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: 0.28"
Excluding outliers - 931 stars left (next iteration limit 1024)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits -region wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.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.ads0c5eYRE (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_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.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_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits
WCS_IMAGE_NAME=wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits
WCS-calibrated image found: wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits
Checking if the catalog wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits.cat corresponding to the image wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits alredy exist and is non-empty...
Catalog wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits.cat corresponding to the image wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits
WCS catalog name: wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=966, passed=27829
Got 27829 stars (including 26828 good ones) from the SExtractor catalog wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits.cat
util/solve_plate_with_UCAC5 got 27829 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 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 922 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: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
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 922 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.42"
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 922 stars left (next iteration limit 1014)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits -region wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.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.xpy1YEDVDN (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_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.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_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits
WCS_IMAGE_NAME=wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits
WCS-calibrated image found: wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits
Checking if the catalog wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits.cat corresponding to the image wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits alredy exist and is non-empty...
Catalog wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits.cat corresponding to the image wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits
WCS catalog name: wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=943, passed=27601
Got 27601 stars (including 26626 good ones) from the SExtractor catalog wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits.cat
util/solve_plate_with_UCAC5 got 27601 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 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 924 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: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
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 924 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.41"
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 924 stars left (next iteration limit 1016)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits -region wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.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_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.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_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
Saving fully-calibrated image wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.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_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
Saving fully-calibrated image wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.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_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-03_20.00sec_-15.00C_LIGHT_0038.fits
Saving fully-calibrated image wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.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_2026-03-25_CI_Sex-02-Q2b1x1_011952_TTUQ2b1x1_12579_2qMCBapL/wcs_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039.fits
Preparing the HTML report for the field Sex-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out52217.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52288.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52379.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52387.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52427.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out52350.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 52210_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039
The candidate 52210_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039 did not pass the final checks
**** FOUND 10:08:12.29 -01:06:28.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52216_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039
The candidate 52216_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039 did not pass the final checks
**** FOUND 10:22:24.89 -01:37:48.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52217_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039
The candidate 52217_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039 did not pass the final checks
**** FOUND 10:43:30.16 -03:20:30.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)
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Considering the candidate 52218_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039
The candidate 52218_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039 did not pass the final checks
**** FOUND 10:35:12.95 -00:14:39.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52221_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039
The candidate 52221_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039 did not pass the final checks
**** FOUND 10:41:25.63 -02:06:56.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52222_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039
The candidate 52222_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039 did not pass the final checks
**** FOUND 09:56:43.19 -04:04:07.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52248_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039
The candidate 52248_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039 did not pass the final checks
**** FOUND 10:42:50.63 +00:24:40.1 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52273_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039
The candidate 52273_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039 did not pass the final checks
**** FOUND 10:08:28.93 -03:29:25.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52283_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039
The candidate 52283_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039 did not pass the final checks
**** FOUND 10:25:43.88 +01:28:08.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52288_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039
The candidate 52288_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039 did not pass the final checks
**** FOUND 10:07:40.05 +00:53:47.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 1.349 3834935238711438336 151.91715311663 +00.89624903413 12.2095 11.7225 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.349#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52298_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039
The candidate 52298_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039 did not pass the final checks
**** FOUND 10:34:35.91 +01:46:35.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52313_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039
The candidate 52313_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039 did not pass the final checks
**** FOUND 10:27:13.43 -04:56:55.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52350_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039
Preparing report for the candidate 52350_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039
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Considering the candidate 52352_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039
The candidate 52352_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039 did not pass the final checks
**** FOUND 10:26:49.68 -00:07:32.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52357_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039
The candidate 52357_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039 did not pass the final checks
**** FOUND 10:20:55.77 +01:55:06.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52370_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039
The candidate 52370_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (19.0") between the two second-epoch detections
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Considering the candidate 52373_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039
The candidate 52373_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039 did not pass the final checks
**** FOUND 10:32:05.27 -05:48:44.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52379_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039
The candidate 52379_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039 did not pass the final checks
**** FOUND 09:56:46.03 -02:18:20.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 0.569 3829563132272400384 149.19175868300 -02.30573790444 13.4767 13.0381 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.569#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52381_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039
The candidate 52381_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039 did not pass the final checks
**** FOUND 09:54:07.33 -03:32:45.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52385_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039
The candidate 52385_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 52387_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039
The candidate 52387_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039 did not pass the final checks
**** FOUND 10:18:20.56 -03:53:06.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 1.652 3780335552860135936 154.58583873087 -03.88550897095 13.6567 13.2234 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.652#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52388_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039
The candidate 52388_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039 did not pass the final checks
**** FOUND 10:11:40.85 +02:12:34.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52391_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039
The candidate 52391_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039 did not pass the final checks
**** FOUND 10:04:12.62 -00:03:00.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52395_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039
The candidate 52395_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039 did not pass the final checks
**** FOUND 10:41:13.19 -00:17:32.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52396_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039
The candidate 52396_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039 did not pass the final checks
**** FOUND 10:16:46.01 -03:07:19.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52427_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039
The candidate 52427_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039 did not pass the final checks
**** FOUND 10:10:19.16 -05:01:30.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.83, MAG_FAINT_SEARCH_LIMIT=14.81)GAIADR2_OUTPUT=# 1.848 3779954301498700672 152.58034285533 -05.02524313865 13.9766 13.5175 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.848#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52436_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039
The candidate 52436_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039 did not pass the final checks
**** FOUND 10:27:39.36 -00:56:38.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52453_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039
The candidate 52453_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039 did not pass the final checks
**** FOUND 10:18:18.88 -01:13:36.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52465_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039
The candidate 52465_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039 did not pass the final checks
**** FOUND 10:01:36.03 +01:07:36.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52472_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039
The candidate 52472_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039 did not pass the final checks
**** FOUND 10:18:36.42 +01:34:19.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34331_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039
The candidate 34331_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 12839_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039
The candidate 12839_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039 did not pass the final checks
**** FOUND 10:34:55.96 -00:20:33.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21480_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039
The candidate 21480_fd_Sex-02-Q2b1x1_2026-03-25_01-14-57_20.00sec_-14.90C_LIGHT_0039 did not pass the final checks