This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.6311,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260227.1311 13.46CV 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/Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:40:28.19 +27:34:03.7 ;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_Tri-01-Q1b1x1_2025-12-22_23-05-47_20_00sec_-15_00C_LIGHT_0216_fits__*pix.png resample_wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20_00sec_-15_00C_LIGHT_0216_fits__*pix.png resample_wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20_00sec_-15_00C_LIGHT_0216_fits__*pix.png resample_wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20_00sec_-15_00C_LIGHT_0216_fits__*pix.png resample_wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20_00sec_-15_00C_LIGHT_0077_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 27.1311* 01 51 51.14 +30 53 52.7 14.3 U Tri 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,2461098.6311,14.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260227.1311 14.31CV 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/Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:51:51.14 +30:53:52.7 ;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_Tri-01-Q1b1x1_2025-12-22_23-05-47_20_00sec_-15_00C_LIGHT_0216_fits__*pix.png resample_wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20_00sec_-14_90C_LIGHT_0078_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20_00sec_-15_00C_LIGHT_0216_fits__*pix.png resample_wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20_00sec_-15_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20_00sec_-15_00C_LIGHT_0216_fits__*pix.png resample_wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20_00sec_-14_90C_LIGHT_0078_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20_00sec_-15_00C_LIGHT_0216_fits__*pix.png resample_wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20_00sec_-15_00C_LIGHT_0077_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: 2461032.71246903 23.12.2025 05:05:47.324 /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits
First image: 2461032.71246903 23.12.2025 05:05:47.324 /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits
Last image: 2461098.63144818 27.02.2026 03:09:07.123 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.53
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 11603
Objects passed selection criteria: 11570
Measurements per detected object (mean, median, min, max): 3.1 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 3.0 2 4
Average stars detected per image: 9190.75
Average stars matched: 9030 (98.251 %)
Memory usage VmPeak: 117380 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Feb 26 21:11:01 CST 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.71246903 23.12.2025 05:05:47.324 /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits
First image: 2461032.71246903 23.12.2025 05:05:47.324 /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits
Last image: 2461098.63144818 27.02.2026 03:09:07.123 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 44
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.28
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 15 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 67208
Objects passed selection criteria: 67108
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 57121.5
Average stars matched: 55607 (97.3486 %)
Memory usage VmPeak: 166756 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Feb 26 21:12:07 CST 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits
SExtractor catalog cache: saved Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits.cat to cache
SExtractor catalog cache: saved Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.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/Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.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: 2461098.63070286
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_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits exists and is non-empty
Saving wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits to local_wcs_cache/
'wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits' -> 'local_wcs_cache/wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits'
wcs_Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits exists and is non-empty
Saving wcs_Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits to local_wcs_cache/
'wcs_Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits' -> 'local_wcs_cache/wcs_Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits'
wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits exists and is non-empty
Saving wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits to local_wcs_cache/
'wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits' -> 'local_wcs_cache/wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits'
wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits exists and is non-empty
Saving wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits to local_wcs_cache/
'wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits' -> 'local_wcs_cache/wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.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 01:59:59.700 +29:59:49.23
Second-epoch image center 01:59:59.392 +30:00:06.85
Angular distance between the image centers 0.01 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:59:59.700 +29:59:49.23
Second-epoch image center 02:00:02.512 +30:00:39.19
Angular distance between the image centers 0.02 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 01:59:59.392 +30:00:06.85
Second-epoch second image center 02:00:02.512 +30:00:39.19
Angular distance between the image centers 0.01440 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/Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits &> /tmp/tmp.AKsq9vxEs9
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits &> /tmp/tmp.IA0S7fq3x0
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits &> /tmp/tmp.UxXnw7G9Hy
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits &> /tmp/tmp.dHAppuYU0t
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits
Calibrating the magnitude scale
Found non-empty wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.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_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits and wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.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_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits and wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits.cat
Found non-empty wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits and wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits.cat
The reference image (wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits) and catalog (wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits.cat) found
'wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.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 6798 out of 12398 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.927134
a=0.000000 b=1.000000 c=22.927134
From vast_summary.log: estimated ref. image limiting mag.: -7.53
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.40
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.40
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits
2.0 pix Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits
2.0 pix fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits
2.0 pix fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits
Limiting magnitude estimates:
15.4 mag. Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits
15.4 mag. Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits
14.5 mag. fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits
14.5 mag. fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 11.5 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.AKsq9vxEs9 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits' -> 'wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits
WCS_IMAGE_NAME=wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits
WCS-calibrated image found: wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits
Checking if the catalog wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits.cat corresponding to the image wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits alredy exist and is non-empty...
Catalog wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits.cat corresponding to the image wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits
WCS catalog name: wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=937, passed=12398
Got 12398 stars (including 11445 good ones) from the SExtractor catalog wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits.cat
util/solve_plate_with_UCAC5 got 12398 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 958 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: 0.30"
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 958 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: 0.29"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits -region wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.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.IA0S7fq3x0 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits' -> 'wcs_Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits
WCS_IMAGE_NAME=wcs_Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits
WCS-calibrated image found: wcs_Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits
Checking if the catalog wcs_Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits.cat corresponding to the image wcs_Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits alredy exist and is non-empty...
Catalog wcs_Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits.cat corresponding to the image wcs_Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits
WCS catalog name: wcs_Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=935, passed=12279
Got 12279 stars (including 11329 good ones) from the SExtractor catalog wcs_Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits.cat
util/solve_plate_with_UCAC5 got 12279 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
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 958 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: 0.31"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits -region wcs_Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.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.UxXnw7G9Hy (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits
WCS_IMAGE_NAME=wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits
WCS-calibrated image found: wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits
Checking if the catalog wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits.cat corresponding to the image wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits alredy exist and is non-empty...
Catalog wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits.cat corresponding to the image wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits
WCS catalog name: wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=546, passed=6165
Got 6165 stars (including 5610 good ones) from the SExtractor catalog wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits.cat
util/solve_plate_with_UCAC5 got 6165 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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 952 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: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits -region wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.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.dHAppuYU0t (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits
WCS_IMAGE_NAME=wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits
WCS-calibrated image found: wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits
Checking if the catalog wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits.cat corresponding to the image wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits alredy exist and is non-empty...
Catalog wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits.cat corresponding to the image wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits
WCS catalog name: wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=575, passed=6167
Got 6167 stars (including 5586 good ones) from the SExtractor catalog wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits.cat
util/solve_plate_with_UCAC5 got 6167 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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 954 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: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits -region wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits'
Saving fully-calibrated image wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits'
Preparing the HTML report for the field Tri-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20626_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078
The candidate 20626_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078 did not pass the final checks
**** FOUND 01:49:30.85 +28:41:55.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11845_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078
The candidate 11845_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078 did not pass the final checks
**** FOUND 02:16:07.13 +25:03:24.3 in the exclusion list exclusion_list_tycho2.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Tri-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits
SExtractor catalog cache: saved Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits.cat to cache
SExtractor catalog cache: saved Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits
Creating symlink local_wcs_cache/wcs_Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits
Creating symlink local_wcs_cache/wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits
Creating symlink local_wcs_cache/wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.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_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits exists and is non-empty
wcs_Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits exists and is non-empty
wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits exists and is non-empty
wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.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 01:59:59.700 +29:59:49.23
Second-epoch image center 01:59:59.392 +30:00:06.85
Angular distance between the image centers 0.01 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:59:59.700 +29:59:49.23
Second-epoch image center 02:00:02.512 +30:00:39.19
Angular distance between the image centers 0.02 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 01:59:59.392 +30:00:06.85
Second-epoch second image center 02:00:02.512 +30:00:39.19
Angular distance between the image centers 0.01440 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/Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits &> /tmp/tmp.tLWQpFl18c
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits &> /tmp/tmp.346Rcmquag
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits &> /tmp/tmp.lKSWrLNfyq
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits &> /tmp/tmp.rZUwuCHr0D
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits
Calibrating the magnitude scale
Found non-empty wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.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_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits and wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.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_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits and wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits.cat
Found non-empty wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits and wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits.cat
The reference image (wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits) and catalog (wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits.cat) found
'wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.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 6891 out of 72042 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.818549
a=0.000000 b=1.000000 c=22.818549
From vast_summary.log: estimated ref. image limiting mag.: -7.28
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.54
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.54
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 43 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits
1.9 pix Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits
1.9 pix fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits
1.9 pix fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits
Limiting magnitude estimates:
15.5 mag. Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits
15.6 mag. Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits
14.6 mag. fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits
14.6 mag. fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits
All-image limiting magnitude estimate: 14.6 (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 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.tLWQpFl18c (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits' -> 'wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits
WCS_IMAGE_NAME=wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits
WCS-calibrated image found: wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits
Checking if the catalog wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits.cat corresponding to the image wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits alredy exist and is non-empty...
Catalog wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits.cat corresponding to the image wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits
WCS catalog name: wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=23, blended=4578, passed=72019
Got 72019 stars (including 67304 good ones) from the SExtractor catalog wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits.cat
util/solve_plate_with_UCAC5 got 72019 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 955 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 955 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: 0.30"
Excluding outliers - 955 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits -region wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tri-01-Q1b1x1_2025-12-22_23-05-47_20.00sec_-15.00C_LIGHT_0216.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.346Rcmquag (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits' -> 'wcs_Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits
WCS_IMAGE_NAME=wcs_Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits
WCS-calibrated image found: wcs_Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits
Checking if the catalog wcs_Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits.cat corresponding to the image wcs_Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits alredy exist and is non-empty...
Catalog wcs_Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits.cat corresponding to the image wcs_Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits
WCS catalog name: wcs_Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=22, blended=4604, passed=72991
Got 72991 stars (including 68246 good ones) from the SExtractor catalog wcs_Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits.cat
util/solve_plate_with_UCAC5 got 72991 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 956 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: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits -region wcs_Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tri-01-Q1b1x1_2025-12-22_23-06-23_20.00sec_-15.00C_LIGHT_0217.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.lKSWrLNfyq (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits
WCS_IMAGE_NAME=wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits
WCS-calibrated image found: wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits
Checking if the catalog wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits.cat corresponding to the image wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits alredy exist and is non-empty...
Catalog wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits.cat corresponding to the image wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits
WCS catalog name: wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=1711, passed=42568
Got 42568 stars (including 40776 good ones) from the SExtractor catalog wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits.cat
util/solve_plate_with_UCAC5 got 42568 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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 953 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: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 953 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits -region wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.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.rZUwuCHr0D (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits
WCS_IMAGE_NAME=wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits
WCS-calibrated image found: wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits
Checking if the catalog wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits.cat corresponding to the image wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits alredy exist and is non-empty...
Catalog wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits.cat corresponding to the image wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits
WCS catalog name: wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=1759, passed=42349
Got 42349 stars (including 40506 good ones) from the SExtractor catalog wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits.cat
util/solve_plate_with_UCAC5 got 42349 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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 953 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: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 953 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits -region wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-08-02_20.00sec_-15.00C_LIGHT_0077.fits
Saving fully-calibrated image wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Tri-01-Q1b1x1_210950_TTUQ1b1x1_18810_qCs0QhP9/wcs_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078.fits
Preparing the HTML report for the field Tri-01-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out87682.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out87685.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out87718.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out87723.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out87725.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out87728.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out87741.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out87746.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out87748.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out87754.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out87757.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out87762.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out87767.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out87768.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out87770.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out87775.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out87783.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out87788.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out87826.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out87717.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out87858.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: 1s
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Considering the candidate 87610_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078
The candidate 87610_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078 did not pass the final checks
**** FOUND 02:05:46.32 +33:24:48.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 87612_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078
The candidate 87612_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078 did not pass the final checks
**** FOUND 01:51:41.84 +30:19:45.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 87615_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078
The candidate 87615_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078 did not pass the final checks
**** FOUND 02:14:20.95 +34:12:08.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 87617_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078
The candidate 87617_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078 did not pass the final checks
**** FOUND 02:09:22.74 +28:22:10.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 87619_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078
The candidate 87619_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078 did not pass the final checks
**** FOUND 02:08:46.47 +30:31:25.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 87654_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078
The candidate 87654_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078 did not pass the final checks
**** FOUND 02:17:29.80 +33:50:10.6 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 87655_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078
The candidate 87655_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078 did not pass the final checks
**** FOUND 01:29:18.74 +25:15:28.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 87657_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078
The candidate 87657_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078 did not pass the final checks
**** FOUND 02:06:55.98 +25:41:41.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 87671_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078
The candidate 87671_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078 did not pass the final checks
**** FOUND 02:25:01.80 +33:53:25.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 87680_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078
The candidate 87680_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078 did not pass the final checks
**** FOUND 01:41:38.23 +33:19:30.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 87682_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078
The candidate 87682_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078 did not pass the final checks
**** FOUND 01:50:38.86 +27:55:42.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 0.723 299016967473031936 027.66199619269 +27.92868801462 12.9612 12.3477 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.723#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 87685_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078
The candidate 87685_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078 did not pass the final checks
**** FOUND 02:22:08.57 +30:20:24.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 1.458 131999982982961920 035.53544531517 +30.34033531946 12.9456 12.2550 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.458#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 87694_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078
The candidate 87694_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078 did not pass the final checks
**** FOUND 01:27:04.92 +34:39:32.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 87701_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078
The candidate 87701_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078 did not pass the final checks
**** FOUND 02:27:19.69 +32:43:04.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 87702_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078
The candidate 87702_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078 did not pass the final checks
**** FOUND 01:31:49.99 +28:50:27.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 87707_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078
The candidate 87707_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078 did not pass the final checks
**** FOUND 01:28:57.68 +34:55:58.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 87717_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078
Preparing report for the candidate 87717_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078
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Considering the candidate 87718_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078
The candidate 87718_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078 did not pass the final checks
**** FOUND 02:20:15.22 +29:48:11.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 1.373 131867113874576768 035.06373429328 +29.80343010783 13.5054 12.8258 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.373#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 87723_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078
The candidate 87723_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078 did not pass the final checks
**** FOUND 01:28:18.24 +30:34:30.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 3.171 315328634788023680 022.07586471287 +30.57587306250 13.5357 12.9032 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.171#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 87725_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078
The candidate 87725_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078 did not pass the final checks
**** FOUND 01:55:04.21 +27:16:03.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 1.334 298164193126554240 028.76738408468 +27.26789872443 13.4420 12.8459 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.334#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 87726_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078
The candidate 87726_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078 did not pass the final checks
**** FOUND 02:01:10.69 +25:11:19.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 87728_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078
The candidate 87728_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078 did not pass the final checks
**** FOUND 02:03:34.28 +25:10:49.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 0.763 105305799165397760 030.89278944427 +25.18012504406 13.6335 13.0788 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.763#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 87734_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078
The candidate 87734_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078 did not pass the final checks
**** FOUND 02:09:18.54 +33:55:27.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 87741_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078
The candidate 87741_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078 did not pass the final checks
**** FOUND 02:19:23.21 +28:48:13.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 2.501 107729363311368704 034.84594426749 +28.80367573648 13.8341 13.2791 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.501#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 87746_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078
The candidate 87746_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078 did not pass the final checks
**** FOUND 01:28:15.71 +30:34:29.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 2.109 315328806586715648 022.06513097822 +30.57537471362 13.6484 13.1820 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.109#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 87748_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078
The candidate 87748_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078 did not pass the final checks
**** FOUND 01:58:08.44 +31:05:53.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)GAIADR2_OUTPUT=# 4.073 301169841304530048 029.53518113166 +31.09703538491 13.7392 13.1528 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.073#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 87754_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078
The candidate 87754_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078 did not pass the final checks
**** FOUND 01:50:34.41 +27:57:42.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 1.114 299018101344393216 027.64328679468 +27.96207720559 13.6015 13.0445 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.114#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 87757_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078
The candidate 87757_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078 did not pass the final checks
**** FOUND 01:45:38.86 +34:16:47.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 2.052 317706637920794880 026.41256171696 +34.28011886129 14.1392 13.6299 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.052#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 87762_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078
The candidate 87762_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078 did not pass the final checks
**** FOUND 01:47:49.41 +28:03:19.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 0.476 298846062134444160 026.95587362006 +28.05536787638 13.8931 13.4158 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.476#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 87766_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078
The candidate 87766_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078 did not pass the final checks
**** FOUND 02:11:10.74 +25:57:59.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 87767_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078
The candidate 87767_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078 did not pass the final checks
**** FOUND 02:22:36.80 +31:31:44.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 0.520 132662507457960960 035.65341297342 +31.52895581563 13.7030 13.1710 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.520#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 87768_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078
The candidate 87768_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078 did not pass the final checks
**** FOUND 02:14:02.75 +34:38:12.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 2.305 326394051090932736 033.51113573303 +34.63738811801 13.7315 13.1266 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.305#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 87769_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078
The candidate 87769_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078 did not pass the final checks
**** FOUND 02:28:18.72 +29:40:31.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 87770_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078
The candidate 87770_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078 did not pass the final checks
**** FOUND 02:01:57.68 +29:52:25.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 2.214 300797557834814848 030.48963802314 +29.87354510326 14.0982 13.5859 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.214#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 87772_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078
The candidate 87772_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078 did not pass the final checks
**** FOUND 02:03:42.74 +25:54:47.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 87775_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078
The candidate 87775_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078 did not pass the final checks
**** FOUND 02:02:23.64 +29:44:15.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 1.224 300792094636423936 030.59812023716 +29.73763835863 14.0474 13.5824 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.224#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 87778_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078
The candidate 87778_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078 did not pass the final checks
**** FOUND 01:39:26.28 +27:11:36.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 87783_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078
The candidate 87783_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078 did not pass the final checks
**** FOUND 01:49:19.36 +32:26:18.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 1.419 305279923144042240 027.33037536412 +32.43880797165 14.0879 13.5638 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.419#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 87788_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078
The candidate 87788_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078 did not pass the final checks
**** FOUND 02:20:16.17 +27:52:21.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 3.507 106901121817998720 035.06785426296 +27.87348838904 14.1517 13.5729 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.507#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 87822_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078
The candidate 87822_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078 did not pass the final checks
**** FOUND 02:14:26.87 +27:56:38.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 87826_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078
The candidate 87826_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078 did not pass the final checks
**** FOUND 02:02:13.43 +34:39:21.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 1.476 329256492174806144 030.55633494483 +34.65621281961 14.2198 13.6492 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.476#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 87858_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078
Preparing report for the candidate 87858_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078
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Considering the candidate 50296_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078
The candidate 50296_fd_Tri-01-Q1b1x1_2026-02-26_21-09-07_20.00sec_-14.90C_LIGHT_0078 did not pass the final checks