This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc
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
CSS 140309:102844-161303,2461093.6976,14.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CSS 140309:102844-161303 20260222.1976 14.48CV 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/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:28:43.70 -16:13:02.6 ;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_Hya-09-Q1b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20_00sec_-15_00C_LIGHT_0170_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20_00sec_-15_00C_LIGHT_0169_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20_00sec_-15_00C_LIGHT_0170_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20_00sec_-15_00C_LIGHT_0169_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
ASAS J105356-1350.4,2461093.6976,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J105356-1350.4 20260222.1976 13.36CV 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/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:53:56.11 -13:50:20.9 ;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_Hya-09-Q1b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20_00sec_-15_00C_LIGHT_0170_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20_00sec_-15_00C_LIGHT_0169_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20_00sec_-15_00C_LIGHT_0170_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20_00sec_-15_00C_LIGHT_0169_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.91964973 23.12.2025 10:04:07.737 /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
First image: 2461032.91964973 23.12.2025 10:04:07.737 /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
Last image: 2461093.69787821 22.02.2026 04:44:46.677 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.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.: -7.97
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: 4 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): 7254
Objects passed selection criteria: 7241
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: 6658.5
Average stars matched: 6559.5 (98.5132 %)
Memory usage VmPeak: 113492 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Feb 22 01:47:08 CST 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.91964973 23.12.2025 10:04:07.737 /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
First image: 2461032.91964973 23.12.2025 10:04:07.737 /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
Last image: 2461093.69787821 22.02.2026 04:44:46.677 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 46
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.73
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: 16 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): 44754
Objects passed selection criteria: 44665
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: 42925.8
Average stars matched: 41724.2 (97.201 %)
Memory usage VmPeak: 145320 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Feb 22 01:48:09 CST 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits
SExtractor catalog cache: saved Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat to cache
SExtractor catalog cache: saved Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.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/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.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: 2461093.69739936
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits exists and is non-empty
Saving wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits to local_wcs_cache/
'wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits' -> 'local_wcs_cache/wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits'
wcs_Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits exists and is non-empty
Saving wcs_Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits to local_wcs_cache/
'wcs_Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits' -> 'local_wcs_cache/wcs_Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits'
wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits exists and is non-empty
Saving wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits to local_wcs_cache/
'wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits' -> 'local_wcs_cache/wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits'
wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits exists and is non-empty
Saving wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits to local_wcs_cache/
'wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits' -> 'local_wcs_cache/wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 10:39:59.375 -17:59:54.09
Second-epoch image center 10:40:07.451 -17:59:45.09
Angular distance between the image centers 0.03 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 10:39:59.375 -17:59:54.09
Second-epoch image center 10:40:10.421 -17:59:31.35
Angular distance between the image centers 0.04 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 10:40:07.451 -17:59:45.09
Second-epoch second image center 10:40:10.421 -17:59:31.35
Angular distance between the image centers 0.01237 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/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits &> /tmp/tmp.gn8b7lb3LG
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits &> /tmp/tmp.rqymh5WVxX
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits &> /tmp/tmp.rGTPkmdtdT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits &> /tmp/tmp.vfYVHNN2nS
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.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_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits and wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.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_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits and wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat
Found non-empty wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits and wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat
The reference image (wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits) and catalog (wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat) found
'wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.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 5250 out of 7725 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.887548
a=0.000000 b=1.000000 c=22.887548
From vast_summary.log: estimated ref. image limiting mag.: -7.97
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.92
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.92
____ 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:
2.1 pix Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
2.1 pix Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
2.1 pix fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits
2.1 pix fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits
Limiting magnitude estimates:
14.9 mag. Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
14.9 mag. Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
14.6 mag. fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits
14.6 mag. fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 11.6 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.gn8b7lb3LG (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits' -> 'wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
WCS_IMAGE_NAME=wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
WCS-calibrated image found: wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
Checking if the catalog wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat corresponding to the image wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits alredy exist and is non-empty...
Catalog wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat corresponding to the image wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
WCS catalog name: wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=533, passed=7725
Got 7725 stars (including 7185 good ones) from the SExtractor catalog wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat
util/solve_plate_with_UCAC5 got 7725 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.26"
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: 0.26"
Estimated accuracy of the plate solution: 0.24"
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_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits -region wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.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.rqymh5WVxX (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits' -> 'wcs_Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
WCS_IMAGE_NAME=wcs_Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
WCS-calibrated image found: wcs_Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
Checking if the catalog wcs_Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat corresponding to the image wcs_Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits alredy exist and is non-empty...
Catalog wcs_Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat corresponding to the image wcs_Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
WCS catalog name: wcs_Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=531, passed=7630
Got 7630 stars (including 7093 good ones) from the SExtractor catalog wcs_Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat
util/solve_plate_with_UCAC5 got 7630 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.27"
Estimated accuracy of the plate solution: 0.24"
Excluding outliers - 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_Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits -region wcs_Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.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.rGTPkmdtdT (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits
WCS_IMAGE_NAME=wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits
WCS-calibrated image found: wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits
Checking if the catalog wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits.cat corresponding to the image wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits.cat corresponding to the image wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits
WCS catalog name: wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=492, passed=5716
Got 5716 stars (including 5220 good ones) from the SExtractor catalog wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits.cat
util/solve_plate_with_UCAC5 got 5716 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.1'
Seting catalog search parameters based on the expected field of view 942.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013085 (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 0.010468 (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: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 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_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits -region wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.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.vfYVHNN2nS (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits
WCS_IMAGE_NAME=wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits
WCS-calibrated image found: wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits
Checking if the catalog wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits.cat corresponding to the image wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits.cat corresponding to the image wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits
WCS catalog name: wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=511, passed=5705
Got 5705 stars (including 5187 good ones) from the SExtractor catalog wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits.cat
util/solve_plate_with_UCAC5 got 5705 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.1'
Seting catalog search parameters based on the expected field of view 942.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013085 (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 0.010468 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
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: 0.37"
Estimated accuracy of the plate solution: 0.36"
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_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits -region wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits'
Saving fully-calibrated image wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits'
Preparing the HTML report for the field Hya-09-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20384_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170
The candidate 20384_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170 did not pass the final checks
**** FOUND 10:56:52.05 -20:26:01.3 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Hya-09-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits
SExtractor catalog cache: saved Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat to cache
SExtractor catalog cache: saved Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
Creating symlink local_wcs_cache/wcs_Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.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_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits exists and is non-empty
wcs_Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits exists and is non-empty
wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits exists and is non-empty
wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 10:39:59.375 -17:59:54.09
Second-epoch image center 10:40:07.451 -17:59:45.09
Angular distance between the image centers 0.03 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 10:39:59.375 -17:59:54.09
Second-epoch image center 10:40:10.421 -17:59:31.35
Angular distance between the image centers 0.04 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 10:40:07.451 -17:59:45.09
Second-epoch second image center 10:40:10.421 -17:59:31.35
Angular distance between the image centers 0.01237 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/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits &> /tmp/tmp.uGBR31Iqwr
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits &> /tmp/tmp.2z5A1yriYK
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits &> /tmp/tmp.BosxfD9VVZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits &> /tmp/tmp.16ENQavWtW
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.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_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits and wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.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_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits and wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat
Found non-empty wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits and wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat
The reference image (wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits) and catalog (wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat) found
'wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.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 5627 out of 46060 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.755505
a=0.000000 b=1.000000 c=22.755505
From vast_summary.log: estimated ref. image limiting mag.: -7.73
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.03
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.03
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 41 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
2.0 pix Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
1.9 pix fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits
1.9 pix fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits
Limiting magnitude estimates:
15.0 mag. Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
15.0 mag. Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
14.7 mag. fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits
14.7 mag. fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.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.uGBR31Iqwr (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits' -> 'wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
WCS_IMAGE_NAME=wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
WCS-calibrated image found: wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
Checking if the catalog wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat corresponding to the image wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits alredy exist and is non-empty...
Catalog wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat corresponding to the image wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
WCS catalog name: wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=1888, passed=46057
Got 46057 stars (including 44088 good ones) from the SExtractor catalog wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat
util/solve_plate_with_UCAC5 got 46057 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.27"
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 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.28"
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits -region wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-09-Q1b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.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.2z5A1yriYK (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits' -> 'wcs_Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
WCS_IMAGE_NAME=wcs_Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
WCS-calibrated image found: wcs_Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
Checking if the catalog wcs_Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat corresponding to the image wcs_Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits alredy exist and is non-empty...
Catalog wcs_Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat corresponding to the image wcs_Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
WCS catalog name: wcs_Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=1954, passed=46667
Got 46667 stars (including 44657 good ones) from the SExtractor catalog wcs_Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat
util/solve_plate_with_UCAC5 got 46667 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 963 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: 0.26"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits -region wcs_Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-09-Q1b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.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.BosxfD9VVZ (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits
WCS_IMAGE_NAME=wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits
WCS-calibrated image found: wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits
Checking if the catalog wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits.cat corresponding to the image wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits.cat corresponding to the image wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits
WCS catalog name: wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=1567, passed=39886
Got 39886 stars (including 38240 good ones) from the SExtractor catalog wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits.cat
util/solve_plate_with_UCAC5 got 39886 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.1'
Seting catalog search parameters based on the expected field of view 942.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013085 (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 0.010468 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.36"
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits -region wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.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.16ENQavWtW (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits
WCS_IMAGE_NAME=wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits
WCS-calibrated image found: wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits
Checking if the catalog wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits.cat corresponding to the image wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits.cat corresponding to the image wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits
WCS catalog name: wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=1598, passed=40111
Got 40111 stars (including 38444 good ones) from the SExtractor catalog wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits.cat
util/solve_plate_with_UCAC5 got 40111 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 942.1'
Seting catalog search parameters based on the expected field of view 942.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013085 (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 0.010468 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.40"
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits -region wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-05_20.00sec_-15.00C_LIGHT_0169.fits
Saving fully-calibrated image wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Hya-09-Q1b1x1_224622_TTUQ1b1x1_20552_eITLd8Kc/wcs_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170.fits
Preparing the HTML report for the field Hya-09-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out53712.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53716.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53727.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53732.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53737.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53771.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53801.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53810.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53868.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53876.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53925.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53936.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53971.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54009.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out33877.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53975.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
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 53712_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170
The candidate 53712_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170 did not pass the final checks
**** FOUND 10:39:24.05 -18:34:37.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 1.290 3555321705122647936 159.85043735321 -18.57679811093 14.6529 13.8379 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.290#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53713_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170
The candidate 53713_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170 did not pass the final checks
**** FOUND 10:50:14.06 -16:28:16.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53716_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170
The candidate 53716_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170 did not pass the final checks
**** FOUND 10:26:39.30 -13:57:41.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)GAIADR2_OUTPUT=# 1.631 3752528186534803328 156.66342191242 -13.96109425942 14.2390 13.5685 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.631#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53722_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170
The candidate 53722_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170 did not pass the final checks
**** FOUND 10:45:45.03 -14:58:55.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53725_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170
The candidate 53725_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170 did not pass the final checks
**** FOUND 11:05:17.08 -21:03:46.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53727_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170
The candidate 53727_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170 did not pass the final checks
**** FOUND 10:09:32.64 -19:24:51.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 1.983 5669273753168431616 152.38655715176 -19.41408473483 13.6033 13.1000 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.983#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53729_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170
The candidate 53729_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170 did not pass the final checks
**** FOUND 10:08:20.60 -20:47:49.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53731_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170
The candidate 53731_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170 did not pass the final checks
**** FOUND 10:47:21.43 -19:58:06.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53732_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170
The candidate 53732_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170 did not pass the final checks
**** FOUND 11:04:27.60 -21:18:33.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 0.648 3551148199502129920 166.11511996213 -21.30924767638 13.2117 12.7236 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.648#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53737_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170
The candidate 53737_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170 did not pass the final checks
**** FOUND 11:12:37.04 -22:55:30.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 1.127 3537981307242019840 168.15460657413 -22.92481391436 12.5380 11.7075 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.127#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53738_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170
The candidate 53738_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170 did not pass the final checks
**** FOUND 11:00:53.40 -19:35:20.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53739_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170
The candidate 53739_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170 did not pass the final checks
**** FOUND 10:57:39.02 -12:57:26.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53740_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170
The candidate 53740_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170 did not pass the final checks
**** FOUND 10:08:35.02 -17:04:11.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53741_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170
The candidate 53741_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170 did not pass the final checks
**** FOUND 11:07:17.28 -22:38:30.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53742_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170
The candidate 53742_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170 did not pass the final checks
**** FOUND 10:59:13.15 -17:32:27.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53754_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170
The candidate 53754_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170 did not pass the final checks
**** FOUND 10:56:52.02 -20:26:01.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53758_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170
The candidate 53758_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170 did not pass the final checks
**** FOUND 10:27:59.26 -21:22:51.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53759_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170
The candidate 53759_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170 did not pass the final checks
**** FOUND 11:11:31.82 -22:50:14.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 53771_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170
The candidate 53771_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170 did not pass the final checks
**** FOUND 10:55:50.76 -22:18:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 0.927 3549696672354869120 163.96135266601 -22.30716301197 12.5723 12.1362 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.927#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53801_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170
The candidate 53801_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170 did not pass the final checks
**** FOUND 11:10:27.96 -22:47:57.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 1.830 3538744746269218432 167.61618160030 -22.79972067154 13.4632 12.9208 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.830#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53804_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170
The candidate 53804_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170 did not pass the final checks
**** FOUND 11:00:08.21 -14:03:27.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 53805_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170
The candidate 53805_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170 did not pass the final checks
**** FOUND 10:34:00.64 -17:47:33.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53810_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170
The candidate 53810_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170 did not pass the final checks
**** FOUND 10:20:12.79 -13:51:03.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 0.913 3753237195440268032 155.05346349753 -13.85078107639 13.4826 12.9492 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.913#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53827_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170
The candidate 53827_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170 did not pass the final checks
**** FOUND 10:40:50.16 -13:26:25.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53828_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170
The candidate 53828_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170 did not pass the final checks
**** FOUND 10:45:39.79 -21:10:10.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53865_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170
The candidate 53865_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170 did not pass the final checks
**** FOUND 10:41:40.76 -20:03:47.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53868_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170
The candidate 53868_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170 did not pass the final checks
**** FOUND 10:08:09.67 -15:33:44.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.31, MAG_FAINT_SEARCH_LIMIT=15.29)GAIADR2_OUTPUT=# 0.994 5674397717872216192 152.04046446314 -15.56260924646 14.8380 14.4161 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.994#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53876_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170
The candidate 53876_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170 did not pass the final checks
**** FOUND 10:57:15.36 -17:45:53.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.11, MAG_FAINT_SEARCH_LIMIT=15.09)GAIADR2_OUTPUT=# 1.446 3556227977581543424 164.31362009130 -17.76454750344 13.7847 12.8657 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.446#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53890_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170
The candidate 53890_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170 did not pass the final checks
**** FOUND 11:11:58.40 -19:44:34.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53896_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170
The candidate 53896_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170 did not pass the final checks
**** FOUND 11:02:28.96 -13:51:38.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53898_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170
The candidate 53898_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170 did not pass the final checks
**** FOUND 10:10:59.31 -15:27:00.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53915_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170
The candidate 53915_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170 did not pass the final checks
**** FOUND 10:11:19.67 -14:10:10.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53925_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170
The candidate 53925_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170 did not pass the final checks
**** FOUND 11:03:03.35 -17:57:24.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.35, MAG_FAINT_SEARCH_LIMIT=15.33)GAIADR2_OUTPUT=# 1.604 3553218648616446080 165.76417444382 -17.95649350901 14.3178 13.7159 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.604#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53936_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170
The candidate 53936_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170 did not pass the final checks
**** FOUND 11:04:07.52 -22:24:11.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.36, MAG_FAINT_SEARCH_LIMIT=15.34)
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Considering the candidate 53945_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170
The candidate 53945_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170 did not pass the final checks
**** FOUND 11:07:19.60 -20:08:54.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53963_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170
The candidate 53963_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170 did not pass the final checks
**** FOUND 11:05:42.95 -12:58:13.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53971_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170
The candidate 53971_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170 did not pass the final checks
**** FOUND 10:14:19.56 -22:18:31.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.35, MAG_FAINT_SEARCH_LIMIT=15.33)GAIADR2_OUTPUT=# 1.253 5666209650484907904 153.58149555392 -22.30920907284 14.3276 13.8382 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.253#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53975_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170
Preparing report for the candidate 53975_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170
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Considering the candidate 53992_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170
The candidate 53992_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170 did not pass the final checks
**** FOUND 10:32:08.81 -17:52:11.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54009_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170
The candidate 54009_fd_Hya-09-Q1b1x1_2026-02-21_22-44-46_20.00sec_-15.00C_LIGHT_0170 did not pass the final checks