This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM
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,2461119.6815,9.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260320.1815 9.71CV 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/Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:53:29.73 -17:09:19.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20_00sec_-15_00C_LIGHT_0153_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20_00sec_-14_90C_LIGHT_0152_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20_00sec_-15_00C_LIGHT_0153_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20_00sec_-14_90C_LIGHT_0152_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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
W Crt,2461119.6815,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
W Crt 20260320.1815 10.87CV 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/Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:26:29.60 -17:54:51.9 ;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_Crt-02-Q2b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20_00sec_-15_00C_LIGHT_0153_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20_00sec_-14_90C_LIGHT_0152_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20_00sec_-15_00C_LIGHT_0153_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20_00sec_-14_90C_LIGHT_0491_fits__*pix.png resample_wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20_00sec_-14_90C_LIGHT_0152_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.92829378 18.01.2026 10:16:34.583 /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits
First image: 2461058.92829378 18.01.2026 10:16:34.583 /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits
Last image: 2461119.68181257 20.03.2026 04:21:38.606 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.86
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 2 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 6312
Objects passed selection criteria: 6309
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 5894.25
Average stars matched: 5830.75 (98.9227 %)
Memory usage VmPeak: 112504 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Mar 11 15:05:24 CDT 2026
VaST build number 1.0rc88-349-g45f03b26
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 19 23:40:06 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.92829378 18.01.2026 10:16:34.583 /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits
First image: 2461058.92829378 18.01.2026 10:16:34.583 /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits
Last image: 2461119.68181257 20.03.2026 04:21:38.606 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 59
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.59
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 11 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 39057
Objects passed selection criteria: 38983
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 36526.8
Average stars matched: 35445.8 (97.0405 %)
Memory usage VmPeak: 141092 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Mar 11 15:05:24 CDT 2026
VaST build number 1.0rc88-349-g45f03b26
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 19 23:40:53 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits
SExtractor catalog cache: saved Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits.cat to cache
SExtractor catalog cache: saved Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.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/Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.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: 2461119.68127530
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_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits exists and is non-empty
Saving wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits to local_wcs_cache/
'wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits' -> 'local_wcs_cache/wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits'
wcs_Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits exists and is non-empty
Saving wcs_Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits to local_wcs_cache/
'wcs_Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits' -> 'local_wcs_cache/wcs_Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits'
wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits exists and is non-empty
Saving wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits to local_wcs_cache/
'wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits' -> 'local_wcs_cache/wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits'
wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits exists and is non-empty
Saving wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits to local_wcs_cache/
'wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits' -> 'local_wcs_cache/wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:33:19.914 -18:00:12.97
Second-epoch image center 11:33:21.368 -18:00:13.37
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 11:33:19.914 -18:00:12.97
Second-epoch image center 11:33:19.425 -18:00:38.59
Angular distance between the image centers 0.01 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 11:33:21.368 -18:00:13.37
Second-epoch second image center 11:33:19.425 -18:00:38.59
Angular distance between the image centers 0.01041 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/Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits &> /tmp/tmp.QqtQtgb19H
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits &> /tmp/tmp.b55lPRPw9a
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits &> /tmp/tmp.jR0PsaABMJ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits &> /tmp/tmp.4AER0w5IYr
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits
Calibrating the magnitude scale
Found non-empty wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.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_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits and wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.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_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits and wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits.cat
Found non-empty wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits and wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits.cat
The reference image (wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits) and catalog (wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits.cat) found
'wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.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 4532 out of 6465 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.806021
a=0.000000 b=1.000000 c=22.806021
From vast_summary.log: estimated ref. image limiting mag.: -7.86
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.95
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.95
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits
2.0 pix Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits
2.4 pix fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits
2.5 pix fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits
Limiting magnitude estimates:
14.9 mag. Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits
14.9 mag. Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits
14.5 mag. fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits
14.5 mag. fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 11.7 (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.QqtQtgb19H (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits' -> 'wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits
WCS_IMAGE_NAME=wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits
WCS-calibrated image found: wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits
Checking if the catalog wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits.cat corresponding to the image wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits alredy exist and is non-empty...
Catalog wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits.cat corresponding to the image wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits
WCS catalog name: wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=438, passed=6465
Got 6465 stars (including 6019 good ones) from the SExtractor catalog wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits.cat
util/solve_plate_with_UCAC5 got 6465 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.28"
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits -region wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.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.b55lPRPw9a (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits' -> 'wcs_Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits
WCS_IMAGE_NAME=wcs_Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits
WCS-calibrated image found: wcs_Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits
Checking if the catalog wcs_Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits.cat corresponding to the image wcs_Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits alredy exist and is non-empty...
Catalog wcs_Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits.cat corresponding to the image wcs_Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits
WCS catalog name: wcs_Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=443, passed=6464
Got 6464 stars (including 6013 good ones) from the SExtractor catalog wcs_Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits.cat
util/solve_plate_with_UCAC5 got 6464 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.28"
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits -region wcs_Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.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.jR0PsaABMJ (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits
WCS_IMAGE_NAME=wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits
WCS-calibrated image found: wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits
Checking if the catalog wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits.cat corresponding to the image wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits alredy exist and is non-empty...
Catalog wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits.cat corresponding to the image wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits
WCS catalog name: wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=348, passed=5417
Got 5417 stars (including 5065 good ones) from the SExtractor catalog wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits.cat
util/solve_plate_with_UCAC5 got 5417 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.45"
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits -region wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.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.4AER0w5IYr (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits
WCS_IMAGE_NAME=wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits
WCS-calibrated image found: wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits
Checking if the catalog wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits.cat corresponding to the image wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits alredy exist and is non-empty...
Catalog wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits.cat corresponding to the image wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits
WCS catalog name: wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=349, passed=5377
Got 5377 stars (including 5022 good ones) from the SExtractor catalog wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits.cat
util/solve_plate_with_UCAC5 got 5377 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.47"
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits -region wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.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_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits'
Saving fully-calibrated image wcs_Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/wcs_Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits'
Saving fully-calibrated image wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits'
Saving fully-calibrated image wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits'
Preparing the HTML report for the field Crt-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20202.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20213.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out03456.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20207.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 4s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20202_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153
The candidate 20202_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 11:57:48.05 -16:04:12.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.82, MAG_FAINT_SEARCH_LIMIT=11.80)GAIADR2_OUTPUT=# 1.025 3568831954250179200 179.45050311443 -16.07022218519 10.8820 10.4172 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.025#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20207_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153
Preparing report for the candidate 20207_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20213_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153
The candidate 20213_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 11:49:30.27 -19:11:29.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.35, MAG_FAINT_SEARCH_LIMIT=12.33)GAIADR2_OUTPUT=# 1.052 3543780612603346688 177.37581657556 -19.19155101255 11.5307 11.0759 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.052#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20216_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153
The candidate 20216_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 11:21:16.93 -20:17:09.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03456_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153
Preparing report for the candidate 03456_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 6s
Prepared the HTML report for the field Crt-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
11:26:29.60 -17:54:51.9
11:53:29.73 -17:09:19.8
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits
SExtractor catalog cache: saved Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits.cat to cache
SExtractor catalog cache: saved Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits
Creating symlink local_wcs_cache/wcs_Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits
Creating symlink local_wcs_cache/wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits
Creating symlink local_wcs_cache/wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.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_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits exists and is non-empty
wcs_Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits exists and is non-empty
wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits exists and is non-empty
wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 11:33:19.914 -18:00:12.97
Second-epoch image center 11:33:21.368 -18:00:13.37
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 11:33:19.914 -18:00:12.97
Second-epoch image center 11:33:19.425 -18:00:38.59
Angular distance between the image centers 0.01 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 11:33:21.368 -18:00:13.37
Second-epoch second image center 11:33:19.425 -18:00:38.59
Angular distance between the image centers 0.01041 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/Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits &> /tmp/tmp.BRxppCApXC
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits &> /tmp/tmp.VN1GnDN4JQ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits &> /tmp/tmp.ar6pS7Iz3p
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits &> /tmp/tmp.4V58GvoeWE
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits
Calibrating the magnitude scale
Found non-empty wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.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_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits and wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.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_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits and wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits.cat
Found non-empty wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits and wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits.cat
The reference image (wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits) and catalog (wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits.cat) found
'wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.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 4875 out of 41343 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.664859
a=0.000000 b=1.000000 c=22.664859
From vast_summary.log: estimated ref. image limiting mag.: -7.59
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.07
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.07
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 38 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits
1.9 pix Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits
2.3 pix fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits
2.2 pix fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits
Limiting magnitude estimates:
15.1 mag. Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits
15.1 mag. Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits
14.7 mag. fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits
14.7 mag. fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 14.1 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.BRxppCApXC (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits' -> 'wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits
WCS_IMAGE_NAME=wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits
WCS-calibrated image found: wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits
Checking if the catalog wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits.cat corresponding to the image wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits alredy exist and is non-empty...
Catalog wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits.cat corresponding to the image wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits
WCS catalog name: wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=1602, passed=41333
Got 41333 stars (including 39649 good ones) from the SExtractor catalog wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits.cat
util/solve_plate_with_UCAC5 got 41333 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.29"
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits -region wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.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.VN1GnDN4JQ (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits' -> 'wcs_Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits
WCS_IMAGE_NAME=wcs_Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits
WCS-calibrated image found: wcs_Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits
Checking if the catalog wcs_Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits.cat corresponding to the image wcs_Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits alredy exist and is non-empty...
Catalog wcs_Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits.cat corresponding to the image wcs_Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits
WCS catalog name: wcs_Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=1575, passed=41141
Got 41141 stars (including 39487 good ones) from the SExtractor catalog wcs_Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits.cat
util/solve_plate_with_UCAC5 got 41141 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.29"
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits -region wcs_Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.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.ar6pS7Iz3p (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits
WCS_IMAGE_NAME=wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits
WCS-calibrated image found: wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits
Checking if the catalog wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits.cat corresponding to the image wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits alredy exist and is non-empty...
Catalog wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits.cat corresponding to the image wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits
WCS catalog name: wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=1269, passed=32174
Got 32174 stars (including 30860 good ones) from the SExtractor catalog wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits.cat
util/solve_plate_with_UCAC5 got 32174 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.44"
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits -region wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.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.4V58GvoeWE (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits
WCS_IMAGE_NAME=wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits
WCS-calibrated image found: wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits
Checking if the catalog wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits.cat corresponding to the image wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits alredy exist and is non-empty...
Catalog wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits.cat corresponding to the image wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits
WCS catalog name: wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=1335, passed=32543
Got 32543 stars (including 31164 good ones) from the SExtractor catalog wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits.cat
util/solve_plate_with_UCAC5 got 32543 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 966 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: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.46"
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 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.45"
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits -region wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.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_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/wcs_Crt-02-Q2b1x1_2026-01-18_04-16-34_20.00sec_-14.90C_LIGHT_0491.fits
Saving fully-calibrated image wcs_Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/wcs_Crt-02-Q2b1x1_2026-01-18_04-17-09_20.00sec_-15.00C_LIGHT_0492.fits
Saving fully-calibrated image wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-20-52_20.00sec_-14.90C_LIGHT_0152.fits
Saving fully-calibrated image wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Crt-02-Q2b1x1_233756_TTUQ2b1x1_2587_Nq1t5LzM/wcs_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153.fits
Preparing the HTML report for the field Crt-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out23724.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52880.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52881.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52882.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52884.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52885.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52886.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52893.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52900.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52901.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52903.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52930.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53161.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53168.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53248.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53262.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53285.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53290.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53307.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53334.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53353.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 3s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
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Considering the candidate 52878_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153
The candidate 52878_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 11:42:23.44 -14:35:22.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52880_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153
The candidate 52880_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 11:36:14.94 -21:12:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 0.429 3541618697864929664 174.06212905562 -21.20173894346 13.7260 13.0650 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.429#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52881_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153
The candidate 52881_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 11:02:18.35 -14:38:35.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 0.594 3563651261617473408 165.57641522538 -14.64306268986 13.6050 13.0301 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.594#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52882_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153
The candidate 52882_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 12:04:38.02 -20:52:45.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 1.790 3494410169693351168 181.15870864243 -20.87974914000 13.2750 12.7151 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.790#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52884_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153
The candidate 52884_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 12:01:46.73 -22:17:49.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 3.336 3493409992069104640 180.44565115013 -22.29750751440 13.1655 12.5368 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.336#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52885_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153
The candidate 52885_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 12:04:06.44 -22:08:27.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 3.465 3493428060995768192 181.02580146149 -22.14083050658 12.9640 12.4745 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.465#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52886_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153
The candidate 52886_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 11:51:42.59 -16:46:23.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)
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Considering the candidate 52887_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153
The candidate 52887_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 11:58:58.09 -16:15:33.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52889_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153
The candidate 52889_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 52890_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153
The candidate 52890_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 11:16:00.77 -21:11:13.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52893_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153
The candidate 52893_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 12:05:30.34 -22:48:21.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 4.512 3493136248033402624 181.37530112081 -22.80654967893 12.3587 11.6409 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.512#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52894_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153
The candidate 52894_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 11:44:28.50 -19:46:36.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52900_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153
The candidate 52900_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 11:51:29.81 -17:55:12.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 0.116 3544024974765612288 177.87419185613 -17.92019415955 12.6353 12.1388 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.116#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52901_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153
The candidate 52901_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 12:04:58.90 -21:34:53.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 4.094 3493552722422158336 181.24663363445 -21.58172462477 11.9606 11.2775 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.094#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52903_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153
The candidate 52903_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 11:54:35.06 -18:55:35.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.50, MAG_FAINT_SEARCH_LIMIT=13.48)GAIADR2_OUTPUT=# 0.844 3543099907529526144 178.64585902297 -18.92673853663 12.2745 11.7377 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.844#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52908_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153
The candidate 52908_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 11:53:29.74 -17:09:19.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52930_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153
The candidate 52930_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 11:53:30.49 -16:05:57.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.25, MAG_FAINT_SEARCH_LIMIT=13.23)GAIADR2_OUTPUT=# 0.717 3568523472519053440 178.37719833364 -16.09906410315 12.3538 11.7302 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.717#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53023_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153
The candidate 53023_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 11:21:43.93 -22:07:25.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53029_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153
The candidate 53029_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 11:10:50.18 -13:05:38.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53049_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153
The candidate 53049_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 11:55:43.32 -18:19:02.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53050_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153
The candidate 53050_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 11:46:32.53 -23:05:02.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53058_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153
The candidate 53058_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 11:46:43.96 -21:28:31.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53102_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153
The candidate 53102_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 11:35:56.81 -18:28:47.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53117_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153
The candidate 53117_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 11:54:21.64 -13:39:59.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53161_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153
The candidate 53161_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 11:41:31.07 -20:51:57.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 2.558 3541700302243588352 175.38006360978 -20.86637451575 14.0277 13.4985 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.558#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53165_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153
The candidate 53165_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 11:43:17.41 -17:23:03.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53166_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153
The candidate 53166_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 11:42:53.58 -19:41:50.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53168_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153
The candidate 53168_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 11:40:05.71 -20:44:24.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 1.417 3541741121612663296 175.02404502301 -20.74050870203 14.0018 13.3502 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.417#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53248_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153
The candidate 53248_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 11:52:02.77 -14:00:51.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.11, MAG_FAINT_SEARCH_LIMIT=15.09)GAIADR2_OUTPUT=# 2.105 3572333933144019072 178.01095989660 -14.01401432351 14.3179 13.7958 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.105#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53262_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153
The candidate 53262_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 11:36:13.56 -17:51:23.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.45, MAG_FAINT_SEARCH_LIMIT=15.43)GAIADR2_OUTPUT=# 1.457 3547077463858857216 174.05633379517 -17.85676138220 14.7166 14.2104 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.457#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53285_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153
The candidate 53285_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 11:51:06.20 -15:18:33.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)GAIADR2_OUTPUT=# 1.939 3571625985094776064 177.77538916850 -15.30900709041 14.3867 13.4994 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.939#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53290_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153
The candidate 53290_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 11:41:03.74 -21:09:14.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)GAIADR2_OUTPUT=# 2.133 3541668141528464896 175.26573684898 -21.15345290447 14.2864 13.7082 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.133#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53307_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153
The candidate 53307_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 11:43:18.85 -19:38:06.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.45, MAG_FAINT_SEARCH_LIMIT=15.43)GAIADR2_OUTPUT=# 1.494 3543342354140194176 175.82838277119 -19.63464070520 14.8308 14.3276 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.494#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53334_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153
The candidate 53334_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 11:58:11.08 -18:16:59.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.32, MAG_FAINT_SEARCH_LIMIT=15.30)GAIADR2_OUTPUT=# 0.576 3567185882263455104 179.54599825416 -18.28319703782 14.2816 13.4963 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.576#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53353_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153
The candidate 53353_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 11:50:07.42 -15:18:15.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.50, MAG_FAINT_SEARCH_LIMIT=15.48)GAIADR2_OUTPUT=# 0.383 3571813623625697280 177.53080632716 -15.30416841754 14.5165 13.9289 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.383#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 23724_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153
The candidate 23724_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 12:01:06.11 -17:25:02.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)GAIADR2_OUTPUT=# 5.530 3567340020049534080 180.27698844502 -17.41679986708 11.8895 10.1871 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.530#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 06975_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153
The candidate 06975_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks
**** FOUND 11:09:59.73 -21:22:00.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21796_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153
The candidate 21796_fd_Crt-02-Q2b1x1_2026-03-19_23-21-38_20.00sec_-15.00C_LIGHT_0153 did not pass the final checks