This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461124.7436,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260325.2436 11.13CV 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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:53:41.42 +07:10:39.0 ;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-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20_00sec_-14_90C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20_00sec_-15_00C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20_00sec_-15_00C_LIGHT_0012_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
VARIABLE_NAME,2461124.7436,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260325.2436 13.19CV 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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:41:04.60 +05:05:04.5 ;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-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20_00sec_-14_90C_LIGHT_0013_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20_00sec_-15_00C_LIGHT_0012_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20_00sec_-14_90C_LIGHT_0013_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20_00sec_-15_00C_LIGHT_0482_fits__*pix.png resample_wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20_00sec_-15_00C_LIGHT_0012_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: 2461032.88786619 23.12.2025 09:18:21.639 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
First image: 2461032.88786619 23.12.2025 09:18:21.639 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Last image: 2461124.74393193 25.03.2026 05:51:05.719 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.63
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): 11695
Objects passed selection criteria: 11670
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 9480
Average stars matched: 9319.5 (98.307 %)
Memory usage VmPeak: 118256 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Mar 25 00:56:50 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.88786619 23.12.2025 09:18:21.639 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
First image: 2461032.88786619 23.12.2025 09:18:21.639 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Last image: 2461124.74393193 25.03.2026 05:51:05.719 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 89
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.35
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: 28 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): 70112
Objects passed selection criteria: 69957
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 59947
Average stars matched: 58430.8 (97.4707 %)
Memory usage VmPeak: 1859108 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Mar 25 00:58:24 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits
SExtractor catalog cache: saved Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat to cache
SExtractor catalog cache: saved Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461124.74333898
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits exists and is non-empty
Saving wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits to local_wcs_cache/
'wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits' -> 'local_wcs_cache/wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits'
wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits exists and is non-empty
Saving wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits to local_wcs_cache/
'wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits' -> 'local_wcs_cache/wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits'
wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits exists and is non-empty
Saving wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits to local_wcs_cache/
'wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits' -> 'local_wcs_cache/wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits'
wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits exists and is non-empty
Saving wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits to local_wcs_cache/
'wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits' -> 'local_wcs_cache/wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.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 08:34:18.354 +05:58:52.69
Second-epoch image center 08:34:30.562 +06:02:15.09
Angular distance between the image centers 0.08 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 08:34:18.354 +05:58:52.69
Second-epoch image center 08:34:29.843 +06:02:14.23
Angular distance between the image centers 0.07 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 08:34:30.562 +06:02:15.09
Second-epoch second image center 08:34:29.843 +06:02:14.23
Angular distance between the image centers 0.00299 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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits &> /tmp/tmp.UwFYuxml9a
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits &> /tmp/tmp.nnlA7iBKnI
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits &> /tmp/tmp.kaGn6JQSob
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits &> /tmp/tmp.aAo0XIEn5n
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits and wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits and wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
Found non-empty wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits and wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
The reference image (wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits) and catalog (wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat) found
'wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.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 7589 out of 15650 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.955413
a=0.000000 b=1.000000 c=22.955413
From vast_summary.log: estimated ref. image limiting mag.: -7.63
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.33
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.33
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
2.3 pix Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
2.4 pix fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits
2.5 pix fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits
Limiting magnitude estimates:
15.3 mag. Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
15.3 mag. Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
14.5 mag. fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits
14.4 mag. fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 11.6 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.UwFYuxml9a (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits' -> 'wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WCS_IMAGE_NAME=wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WCS-calibrated image found: wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Checking if the catalog wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat corresponding to the image wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits alredy exist and is non-empty...
Catalog wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat corresponding to the image wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WCS catalog name: wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1186, passed=15650
Got 15650 stars (including 14444 good ones) from the SExtractor catalog wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
util/solve_plate_with_UCAC5 got 15650 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 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
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 953 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: 0.34"
Excluding outliers - 953 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits -region wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.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.nnlA7iBKnI (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.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-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits' -> 'wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WCS_IMAGE_NAME=wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WCS-calibrated image found: wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
Checking if the catalog wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat corresponding to the image wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits alredy exist and is non-empty...
Catalog wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat corresponding to the image wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WCS catalog name: wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1188, passed=15565
Got 15565 stars (including 14349 good ones) from the SExtractor catalog wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat
util/solve_plate_with_UCAC5 got 15565 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 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits -region wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.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.kaGn6JQSob (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits
WCS_IMAGE_NAME=wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits
WCS-calibrated image found: wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits
Checking if the catalog wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits.cat corresponding to the image wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits.cat corresponding to the image wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits
WCS catalog name: wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=536, passed=8646
Got 8646 stars (including 8105 good ones) from the SExtractor catalog wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits.cat
util/solve_plate_with_UCAC5 got 8646 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.60"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.61"
Estimated accuracy of the plate solution: 0.65"
Excluding outliers - 949 stars left (next iteration limit 1043)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits -region wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.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.aAo0XIEn5n (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits
WCS_IMAGE_NAME=wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits
WCS-calibrated image found: wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits
Checking if the catalog wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits.cat corresponding to the image wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits.cat corresponding to the image wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits
WCS catalog name: wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=524, passed=8274
Got 8274 stars (including 7747 good ones) from the SExtractor catalog wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits.cat
util/solve_plate_with_UCAC5 got 8274 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.62"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.62"
Estimated accuracy of the plate solution: 0.65"
Excluding outliers - 953 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits -region wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.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_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits'
Saving fully-calibrated image wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits'
Saving fully-calibrated image wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits'
Saving fully-calibrated image wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits'
Preparing the HTML report for the field Hya-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out20618.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20607_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 20607_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:35:01.79 +02:59:31.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20618_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
Preparing report for the candidate 20618_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 7s
Prepared the HTML report for the field Hya-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
08:53:41.42 +07:10:39.0
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits
SExtractor catalog cache: saved Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat to cache
SExtractor catalog cache: saved Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Creating symlink local_wcs_cache/wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits exists and is non-empty
wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits exists and is non-empty
wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits exists and is non-empty
wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.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 08:34:18.354 +05:58:52.69
Second-epoch image center 08:34:30.562 +06:02:15.09
Angular distance between the image centers 0.08 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 08:34:18.354 +05:58:52.69
Second-epoch image center 08:34:29.843 +06:02:14.23
Angular distance between the image centers 0.07 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 08:34:30.562 +06:02:15.09
Second-epoch second image center 08:34:29.843 +06:02:14.23
Angular distance between the image centers 0.00299 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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits &> /tmp/tmp.puQi4lpXO4
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits &> /tmp/tmp.PxxNfMxiVV
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits &> /tmp/tmp.jPzatY9TYZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits &> /tmp/tmp.HygfTABikz
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits and wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits and wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
Found non-empty wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits and wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
The reference image (wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits) and catalog (wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat) found
'wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.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 7690 out of 90472 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.847783
a=0.000000 b=1.000000 c=22.847783
From vast_summary.log: estimated ref. image limiting mag.: -7.35
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.50
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.50
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 63 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
2.1 pix Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
2.2 pix fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits
2.2 pix fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits
Limiting magnitude estimates:
15.5 mag. Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
15.5 mag. Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
14.7 mag. fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits
14.6 mag. fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 14.1 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.puQi4lpXO4 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.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-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits' -> 'wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WCS_IMAGE_NAME=wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WCS-calibrated image found: wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Checking if the catalog wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat corresponding to the image wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits alredy exist and is non-empty...
Catalog wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat corresponding to the image wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
WCS catalog name: wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=6373, passed=90453
Got 90453 stars (including 83928 good ones) from the SExtractor catalog wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat
util/solve_plate_with_UCAC5 got 90453 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 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 947 stars left (next iteration limit 1041)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits -region wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.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.PxxNfMxiVV (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.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-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits' -> 'wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WCS_IMAGE_NAME=wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WCS-calibrated image found: wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
Checking if the catalog wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat corresponding to the image wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits alredy exist and is non-empty...
Catalog wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat corresponding to the image wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
WCS catalog name: wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=6475, passed=90928
Got 90928 stars (including 84300 good ones) from the SExtractor catalog wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat
util/solve_plate_with_UCAC5 got 90928 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 947 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: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 946 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits -region wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.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.jPzatY9TYZ (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits
WCS_IMAGE_NAME=wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits
WCS-calibrated image found: wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits
Checking if the catalog wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits.cat corresponding to the image wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits.cat corresponding to the image wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits
WCS catalog name: wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=3022, passed=52938
Got 52938 stars (including 49852 good ones) from the SExtractor catalog wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits.cat
util/solve_plate_with_UCAC5 got 52938 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.55"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.55"
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits -region wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.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.HygfTABikz (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits
WCS_IMAGE_NAME=wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits
WCS-calibrated image found: wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits
Checking if the catalog wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits.cat corresponding to the image wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits.cat corresponding to the image wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits
WCS catalog name: wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=2825, passed=50948
Got 50948 stars (including 48064 good ones) from the SExtractor catalog wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits.cat
util/solve_plate_with_UCAC5 got 50948 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.56"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.56"
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 951 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits -region wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.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_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/wcs_Hya-01-Q2b1x1_2025-12-23_03-18-21_20.00sec_-15.00C_LIGHT_0482.fits
Saving fully-calibrated image wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/wcs_Hya-01-Q2b1x1_2025-12-23_03-18-58_20.00sec_-15.00C_LIGHT_0483.fits
Saving fully-calibrated image wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-50-14_20.00sec_-15.00C_LIGHT_0012.fits
Saving fully-calibrated image wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Hya-01-Q2b1x1_005149_TTUQ2b1x1_4376_epyeRWmf/wcs_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013.fits
Preparing the HTML report for the field Hya-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out106064.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106068.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106091.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106094.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106106.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106109.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106112.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106113.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106207.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106236.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106238.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106255.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106256.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106275.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106278.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106282.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106286.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106288.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106291.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106300.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106327.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106329.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106341.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106342.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106365.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106371.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106378.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out106391.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out106259.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 106064_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106064_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:35:12.78 +04:08:20.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.63, MAG_FAINT_SEARCH_LIMIT=15.61)GAIADR2_OUTPUT=# 1.621 3080410987766654592 128.80312741019 +04.13943333386 14.6748 14.2313 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.621#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106068_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106068_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:25:23.67 +07:20:10.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)GAIADR2_OUTPUT=# 0.878 3096992963144524672 126.34861124530 +07.33595089581 14.2778 13.6205 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.878#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106071_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106071_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:25:23.23 +02:16:01.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106077_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106077_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:49:24.89 +02:42:40.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106079_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106079_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 106083_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106083_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:42:52.20 +04:33:34.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106091_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106091_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:33:00.38 +09:08:16.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 0.784 599608500021258624 128.25144676632 +09.13766238405 14.3575 13.8072 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.784#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106094_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106094_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:41:31.71 +04:55:41.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.00, MAG_FAINT_SEARCH_LIMIT=14.98)GAIADR2_OUTPUT=# 1.482 582438560801099776 130.38185796144 +04.92861961740 13.8031 13.2368 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.482#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106097_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106097_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:38:12.64 +03:34:27.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106104_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106104_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:14:53.98 +06:53:42.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106106_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106106_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:18:59.33 +05:22:02.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 0.701 3093360039287389568 124.74738428911 +05.36752975194 13.6955 13.3141 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.701#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106107_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106107_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:58:28.96 +02:32:03.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106108_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106108_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:59:59.50 +02:15:00.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106109_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106109_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:24:41.02 +03:34:08.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 0.542 3092058251879286400 126.17086992368 +03.56928206502 13.5522 13.0050 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.542#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106111_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106111_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:18:44.90 +01:57:54.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106112_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106112_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:14:11.83 +06:10:28.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 2.594 3096664930722266880 123.54886748663 +06.17397141347 13.5678 12.7552 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.594#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106113_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106113_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:37:34.28 +02:09:33.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 1.841 3078765323802264192 129.39233480154 +02.15928176141 13.0220 12.2755 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.841#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106114_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106114_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:28:07.85 +02:49:17.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106116_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106116_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:45:47.91 +04:59:33.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106142_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106142_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:53:41.41 +07:10:38.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 106162_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106162_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:29:00.64 +06:54:44.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106181_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106181_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 106198_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106198_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:37:49.28 +05:42:47.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106203_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106203_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:29:34.51 +08:55:01.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106207_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106207_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:30:59.07 +02:10:23.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 0.663 3079467503711268096 127.74627931662 +02.17323938800 12.8825 12.3052 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.663#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106230_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106230_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:25:01.33 +04:27:40.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106236_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106236_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:28:28.38 +06:57:22.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 0.901 595907578242321536 127.11845050933 +06.95607040551 13.0037 12.4576 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.901#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106238_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106238_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:52:14.65 +04:53:40.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 0.597 581870113289750144 133.06101998362 +04.89441880450 13.0179 12.5406 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.597#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106239_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106239_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:20:27.52 +09:25:25.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106245_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106245_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 106255_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106255_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:49:18.47 +03:42:07.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 1.079 581389313175321984 132.32678571373 +03.70224538489 13.2002 12.4772 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.079#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106256_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106256_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:10:41.29 +02:55:40.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 2.096 3091060582518594176 122.67198047922 +02.92719871375 13.0351 12.4174 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.096#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106259_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
Preparing report for the candidate 106259_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
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Considering the candidate 106260_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106260_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:36:08.65 +02:02:03.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106263_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106263_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 106271_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106271_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:14:21.81 +04:08:07.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106272_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106272_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:55:33.57 +05:55:24.2 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 106275_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106275_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:31:12.14 +06:59:01.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 0.892 595732545439342976 127.80033377685 +06.98371971969 13.4044 12.9381 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.892#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106278_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106278_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:34:39.80 +05:29:12.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 0.806 594758588590537216 128.66604933954 +05.48681256902 13.3709 12.6459 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.806#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106282_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106282_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:26:42.52 +05:13:28.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)GAIADR2_OUTPUT=# 1.114 3093439410282689024 126.67720631324 +05.22497360667 13.3428 12.9406 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.114#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106286_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106286_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:50:24.70 +09:15:34.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 1.536 597593748042459904 132.60309971413 +09.26008096804 13.3421 12.7133 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.536#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106288_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106288_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:22:31.84 +05:01:53.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)GAIADR2_OUTPUT=# 2.640 3093112541795071104 125.63304596815 +05.03212858041 13.4511 12.9737 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.640#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106291_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106291_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:42:21.00 +04:33:39.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 0.794 582221338535393920 130.58766327737 +04.56100986192 13.3032 12.6395 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.794#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106294_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106294_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:11:45.90 +04:15:57.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106298_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106298_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 106300_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106300_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 09:00:59.14 +05:58:35.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 0.844 583448324792360320 135.24664734736 +05.97639553898 13.4675 12.9785 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.844#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106301_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106301_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 106302_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106302_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:53:38.05 +03:04:36.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106303_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106303_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:13:01.92 +04:52:53.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106310_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106310_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:17:45.16 +09:08:45.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106323_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106323_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:23:55.46 +05:08:32.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106327_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106327_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:18:27.80 +04:22:57.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 2.498 3093137800500120704 124.61652267002 +04.38281705845 14.1254 13.6788 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.498#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106329_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106329_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:16:15.97 +05:02:00.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 3.142 3093233492371157504 124.06740052033 +05.03318904787 13.6658 12.9737 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.142#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106341_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106341_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:52:13.35 +06:55:25.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 3.249 584639233324137088 133.05561302649 +06.92465234433 14.0861 13.5517 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.249#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106342_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106342_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:20:49.81 +06:48:50.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 2.346 3096900810326025728 125.20728087593 +06.81348531597 13.8785 13.3868 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.346#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106343_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106343_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 106351_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106351_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:35:47.54 +09:52:45.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106360_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106360_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 106365_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106365_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:38:12.06 +06:23:17.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.92, MAG_FAINT_SEARCH_LIMIT=14.90)GAIADR2_OUTPUT=# 3.082 594914513083324416 129.54938856210 +06.38822687113 14.1825 13.6492 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.082#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106371_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106371_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:24:41.68 +06:08:50.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 3.407 3093758440453413632 126.17287696658 +06.14780613140 14.1773 13.6107 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.407#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106378_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106378_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:34:03.75 +05:41:38.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 0.929 594777894468078080 128.51570999702 +05.69432709755 14.2515 13.7508 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.929#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106391_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 106391_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks
**** FOUND 08:36:02.59 +08:05:36.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 2.732 596457265336567680 129.01004079638 +08.09331948643 14.5492 14.0711 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.732#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78550_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013
The candidate 78550_fd_Hya-01-Q2b1x1_2026-03-25_00-51-05_20.00sec_-14.90C_LIGHT_0013 did not pass the final checks