This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5
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,2461124.7585,9.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260325.2585 9.74CV 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_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:48:55.15 -16:46:53.8 ;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_2026-03-22_01-30-13_20_00sec_-15_00C_LIGHT_0119_fits__*pix.png resample_wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20_00sec_-15_00C_LIGHT_0037_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20_00sec_-15_00C_LIGHT_0119_fits__*pix.png resample_wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20_00sec_-14_90C_LIGHT_0036_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_2026-03-22_01-30-13_20_00sec_-15_00C_LIGHT_0119_fits__*pix.png resample_wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20_00sec_-15_00C_LIGHT_0037_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20_00sec_-15_00C_LIGHT_0119_fits__*pix.png resample_wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20_00sec_-14_90C_LIGHT_0036_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.2585 2461124.7585 13.59 11:46:44.50 -21:28:28.6
283.46480 38.93909 galactic Crt Second-epoch detections are separated by 5.6" and 3.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J176.6947-21.4774 | 11:46:44.50 -21:28:28.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
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
ATO J176.6947-21.4774,2461124.7585,13.59,0.05,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
ATO J176.6947-21.4774 20260325.2585 13.59CV 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_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:46:44.50 -21:28:28.6 ;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_2026-03-22_01-30-13_20_00sec_-15_00C_LIGHT_0119_fits__*pix.png resample_wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20_00sec_-15_00C_LIGHT_0037_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20_00sec_-15_00C_LIGHT_0119_fits__*pix.png resample_wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20_00sec_-14_90C_LIGHT_0036_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_2026-03-22_01-30-13_20_00sec_-15_00C_LIGHT_0119_fits__*pix.png resample_wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20_00sec_-15_00C_LIGHT_0037_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20_00sec_-15_00C_LIGHT_0119_fits__*pix.png resample_wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20_00sec_-14_90C_LIGHT_0036_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: 2461121.77110992 22.03.2026 06:30:13.897 /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits
First image: 2461121.77110992 22.03.2026 06:30:13.897 /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits
Last image: 2461124.75881950 25.03.2026 06:12:32.005 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.85
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): 6369
Objects passed selection criteria: 6344
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 4957
Average stars matched: 4716.5 (95.1483 %)
Memory usage VmPeak: 112412 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Mar 25 01:26:02 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: 2461121.77110992 22.03.2026 06:30:13.897 /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits
First image: 2461121.77110992 22.03.2026 06:30:13.897 /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits
Last image: 2461124.75881950 25.03.2026 06:12:32.005 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 17
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.61
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: 12 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): 36615
Objects passed selection criteria: 36537
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 30356
Average stars matched: 28748.2 (94.7037 %)
Memory usage VmPeak: 138196 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Mar 25 01:26:49 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_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits
SExtractor catalog cache: saved Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits.cat to cache
SExtractor catalog cache: saved Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.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_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461124.75826014
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_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits exists and is non-empty
Saving wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits to local_wcs_cache/
'wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits' -> 'local_wcs_cache/wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits'
wcs_Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits exists and is non-empty
Saving wcs_Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits to local_wcs_cache/
'wcs_Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits' -> 'local_wcs_cache/wcs_Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits'
wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits exists and is non-empty
Saving wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits to local_wcs_cache/
'wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits' -> 'local_wcs_cache/wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits'
wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits exists and is non-empty
Saving wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits to local_wcs_cache/
'wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits' -> 'local_wcs_cache/wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.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 11:33:20.382 -18:00:18.47
Second-epoch image center 11:33:19.056 -18:04:02.31
Angular distance between the image centers 0.06 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 11:33:20.382 -18:00:18.47
Second-epoch image center 11:33:20.940 -18:04:05.05
Angular distance between the image centers 0.06 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 11:33:19.056 -18:04:02.31
Second-epoch second image center 11:33:20.940 -18:04:05.05
Angular distance between the image centers 0.00750 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_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits &> /tmp/tmp.KqpBa4O3DS
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits &> /tmp/tmp.dXFAE8bOrn
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits &> /tmp/tmp.OcV0BND5hT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits &> /tmp/tmp.zS7GsK6mtq
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits
Calibrating the magnitude scale
Found non-empty wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.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_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits and wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.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_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits and wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits.cat
Found non-empty wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits and wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits.cat
The reference image (wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits) and catalog (wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits.cat) found
'wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.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 4663 out of 7181 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.850939
a=0.000000 b=1.000000 c=22.850939
From vast_summary.log: estimated ref. image limiting mag.: -7.85
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.00
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.00
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits
2.2 pix Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits
2.5 pix fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits
2.4 pix fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits
Limiting magnitude estimates:
15.0 mag. Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits
15.0 mag. Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits
14.3 mag. fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits
14.4 mag. fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 11.5 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.KqpBa4O3DS (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_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.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_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.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_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits' -> 'wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits
WCS_IMAGE_NAME=wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits
WCS-calibrated image found: wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits
Checking if the catalog wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits.cat corresponding to the image wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits alredy exist and is non-empty...
Catalog wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits.cat corresponding to the image wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.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_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits
WCS catalog name: wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=429, passed=7181
Got 7181 stars (including 6742 good ones) from the SExtractor catalog wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits.cat
util/solve_plate_with_UCAC5 got 7181 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 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: 0.29"
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 966 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 - 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_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits -region wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.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.dXFAE8bOrn (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_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.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_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.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_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits' -> 'wcs_Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits
WCS_IMAGE_NAME=wcs_Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits
WCS-calibrated image found: wcs_Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits
Checking if the catalog wcs_Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits.cat corresponding to the image wcs_Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits alredy exist and is non-empty...
Catalog wcs_Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits.cat corresponding to the image wcs_Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.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_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits
WCS catalog name: wcs_Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=433, passed=7147
Got 7147 stars (including 6709 good ones) from the SExtractor catalog wcs_Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits.cat
util/solve_plate_with_UCAC5 got 7147 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 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: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 966 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 - 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_Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits -region wcs_Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.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.OcV0BND5hT (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits
WCS_IMAGE_NAME=wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits
WCS-calibrated image found: wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits
Checking if the catalog wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits.cat corresponding to the image wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits alredy exist and is non-empty...
Catalog wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits.cat corresponding to the image wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.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_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits
WCS catalog name: wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=256, passed=4759
Got 4759 stars (including 4498 good ones) from the SExtractor catalog wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits.cat
util/solve_plate_with_UCAC5 got 4759 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.42"
Estimated accuracy of the plate solution: 0.43"
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_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits -region wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.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.zS7GsK6mtq (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits
WCS_IMAGE_NAME=wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits
WCS-calibrated image found: wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits
Checking if the catalog wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits.cat corresponding to the image wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits alredy exist and is non-empty...
Catalog wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits.cat corresponding to the image wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.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_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits
WCS catalog name: wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=266, passed=4655
Got 4655 stars (including 4386 good ones) from the SExtractor catalog wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits.cat
util/solve_plate_with_UCAC5 got 4655 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.50"
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 968 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: 0.48"
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_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits -region wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.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_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits'
Saving fully-calibrated image wcs_Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/wcs_Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits'
Saving fully-calibrated image wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits'
Saving fully-calibrated image wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits'
Preparing the HTML report for the field Crt-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out20361.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20361_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037
Preparing report for the candidate 20361_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037
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 ####
11:48:55.15 -16:46:53.8
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_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits
SExtractor catalog cache: saved Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits.cat to cache
SExtractor catalog cache: saved Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.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_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits
Creating symlink local_wcs_cache/wcs_Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits
Creating symlink local_wcs_cache/wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits
Creating symlink local_wcs_cache/wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.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_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits exists and is non-empty
wcs_Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits exists and is non-empty
wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits exists and is non-empty
wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.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 11:33:20.382 -18:00:18.47
Second-epoch image center 11:33:19.056 -18:04:02.31
Angular distance between the image centers 0.06 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 11:33:20.382 -18:00:18.47
Second-epoch image center 11:33:20.940 -18:04:05.05
Angular distance between the image centers 0.06 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 11:33:19.056 -18:04:02.31
Second-epoch second image center 11:33:20.940 -18:04:05.05
Angular distance between the image centers 0.00750 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_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits &> /tmp/tmp.kGYfp1PqYd
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits &> /tmp/tmp.6xCXLfE3sP
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits &> /tmp/tmp.7JJWUtPIm1
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits &> /tmp/tmp.QkR63e0OnI
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits
Calibrating the magnitude scale
Found non-empty wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.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_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits and wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.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_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits and wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits.cat
Found non-empty wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits and wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits.cat
The reference image (wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits) and catalog (wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits.cat) found
'wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.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 4858 out of 41206 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.741291
a=0.000000 b=1.000000 c=22.741291
From vast_summary.log: estimated ref. image limiting mag.: -7.61
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.13
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.13
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 13 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits
2.1 pix Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits
2.4 pix fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits
2.2 pix fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits
Limiting magnitude estimates:
15.1 mag. Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits
15.1 mag. Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits
14.5 mag. fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits
14.6 mag. fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 14.0 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.kGYfp1PqYd (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_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.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_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.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_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits' -> 'wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits
WCS_IMAGE_NAME=wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits
WCS-calibrated image found: wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits
Checking if the catalog wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits.cat corresponding to the image wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits alredy exist and is non-empty...
Catalog wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits.cat corresponding to the image wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.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_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits
WCS catalog name: wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=1532, passed=41198
Got 41198 stars (including 39610 good ones) from the SExtractor catalog wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits.cat
util/solve_plate_with_UCAC5 got 41198 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 968 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 - 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_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits -region wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.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.6xCXLfE3sP (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_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.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_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.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_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits' -> 'wcs_Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits
WCS_IMAGE_NAME=wcs_Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits
WCS-calibrated image found: wcs_Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits
Checking if the catalog wcs_Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits.cat corresponding to the image wcs_Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits alredy exist and is non-empty...
Catalog wcs_Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits.cat corresponding to the image wcs_Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.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_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits
WCS catalog name: wcs_Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=1543, passed=41399
Got 41399 stars (including 39782 good ones) from the SExtractor catalog wcs_Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits.cat
util/solve_plate_with_UCAC5 got 41399 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.31"
Estimated accuracy of the plate solution: 0.28"
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_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits -region wcs_Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.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.7JJWUtPIm1 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits
WCS_IMAGE_NAME=wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits
WCS-calibrated image found: wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits
Checking if the catalog wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits.cat corresponding to the image wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits alredy exist and is non-empty...
Catalog wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits.cat corresponding to the image wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.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_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits
WCS catalog name: wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=963, passed=27691
Got 27691 stars (including 26699 good ones) from the SExtractor catalog wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits.cat
util/solve_plate_with_UCAC5 got 27691 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.42"
Estimated accuracy of the plate solution: 0.41"
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_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits -region wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.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.QkR63e0OnI (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits
WCS_IMAGE_NAME=wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits
WCS-calibrated image found: wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits
Checking if the catalog wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits.cat corresponding to the image wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits alredy exist and is non-empty...
Catalog wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits.cat corresponding to the image wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.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_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits
WCS catalog name: wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=1037, passed=29068
Got 29068 stars (including 27992 good ones) from the SExtractor catalog wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits.cat
util/solve_plate_with_UCAC5 got 29068 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.50"
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 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.46"
Estimated accuracy of the plate solution: 0.47"
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_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits -region wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.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_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/wcs_Crt-02-Q2b1x1_2026-03-22_01-30-13_20.00sec_-15.00C_LIGHT_0119.fits
Saving fully-calibrated image wcs_Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/wcs_Crt-02-Q2b1x1_2026-03-22_01-31-10_20.00sec_-14.90C_LIGHT_0120.fits
Saving fully-calibrated image wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-11-43_20.00sec_-14.90C_LIGHT_0036.fits
Saving fully-calibrated image wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Crt-02-Q2b1x1_012354_TTUQ2b1x1_13878_Lre9Z5G5/wcs_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037.fits
Preparing the HTML report for the field Crt-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out52658.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52665.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54247.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54359.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54661.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55086.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55831.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55839.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out54957.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 12s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 52658_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037
The candidate 52658_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037 did not pass the final checks
**** FOUND 11:22:13.05 -18:20:47.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 1.351 3546377349830624256 170.55476981412 -18.34647818653 14.3400 13.8412 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.351#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52662_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037
The candidate 52662_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037 did not pass the final checks
**** FOUND 11:16:00.75 -21:11:12.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52665_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037
The candidate 52665_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037 did not pass the final checks
**** FOUND 11:38:11.19 -18:54:18.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 0.380 3546639136676708736 174.54654364815 -18.90506682969 13.0378 12.3282 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.380#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52666_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037
The candidate 52666_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037 did not pass the final checks
**** FOUND 11:25:45.94 -21:36:09.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52775_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037
The candidate 52775_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037 did not pass the final checks
**** FOUND 11:48:55.17 -16:46:53.7 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53943_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037
The candidate 53943_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037 did not pass the final checks
**** FOUND 11:08:51.47 -22:04:01.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54247_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037
The candidate 54247_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037 did not pass the final checks
**** FOUND 11:16:52.51 -18:41:11.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.00, MAG_FAINT_SEARCH_LIMIT=13.98)GAIADR2_OUTPUT=# 1.246 3557908340587096576 169.21895414815 -18.68686546148 13.1149 12.4487 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.246#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54359_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037
The candidate 54359_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037 did not pass the final checks
**** FOUND 11:38:35.85 -21:51:38.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 1.635 3540775784763064576 174.64893670129 -21.86057596598 13.3582 12.9494 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.635#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54661_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037
The candidate 54661_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037 did not pass the final checks
**** FOUND 11:16:28.18 -20:27:02.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 2.750 3539512342824433920 169.11697682278 -20.45013474772 13.4633 12.9806 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.750#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54957_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037
Preparing report for the candidate 54957_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037
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Considering the candidate 55086_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037
The candidate 55086_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037 did not pass the final checks
**** FOUND 11:53:08.98 -15:39:53.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 2.379 3571557368697393792 178.28708847066 -15.66425295088 13.9677 13.5208 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.379#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55831_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037
The candidate 55831_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037 did not pass the final checks
**** FOUND 11:39:53.96 -20:10:44.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.27, MAG_FAINT_SEARCH_LIMIT=15.25)GAIADR2_OUTPUT=# 0.988 3541985075755001600 174.97512208640 -20.17912691413 14.3504 13.8352 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.988#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55839_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037
The candidate 55839_fd_Crt-02-Q2b1x1_2026-03-25_01-12-32_20.00sec_-15.00C_LIGHT_0037 did not pass the final checks