This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I
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
ASAS J105356-1350.4,2461098.7216,13.32,0.05,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
ASAS J105356-1350.4 20260227.2216 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:53:56.16 -13:50:20.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_Hya-09-Q2b1x1_2026-02-26_23-19-17_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_Hya-09-Q2b1x1_2026-02-26_23-18-32_20_00sec_-14_90C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_Hya-09-Q2b1x1_2026-02-26_23-19-17_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_Hya-09-Q2b1x1_2026-02-26_23-18-32_20_00sec_-14_90C_LIGHT_0059_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J102747-1952.8,2461098.7216,11.43,0.05,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
ASAS J102747-1952.8 20260227.2216 11.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:27:47.40 -19:52:51.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_Hya-09-Q2b1x1_2026-02-26_23-19-17_20_00sec_-15_00C_LIGHT_0060_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_Hya-09-Q2b1x1_2026-02-26_23-18-32_20_00sec_-14_90C_LIGHT_0059_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_Hya-09-Q2b1x1_2026-02-26_23-19-17_20_00sec_-15_00C_LIGHT_0060_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_Hya-09-Q2b1x1_2026-02-26_23-18-32_20_00sec_-14_90C_LIGHT_0059_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.91964973 23.12.2025 10:04:07.737 /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
First image: 2461032.91964973 23.12.2025 10:04:07.737 /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
Last image: 2461098.72184932 27.02.2026 05:19:17.781 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.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.: -7.97
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 7247
Objects passed selection criteria: 7225
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: 6254
Average stars matched: 6156.5 (98.441 %)
Memory usage VmPeak: 115788 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Feb 27 02:33:44 CST 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.91964973 23.12.2025 10:04:07.737 /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
First image: 2461032.91964973 23.12.2025 10:04:07.737 /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
Last image: 2461098.72184932 27.02.2026 05:19:17.781 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 52
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.73
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 20 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): 43441
Objects passed selection criteria: 43366
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 39228.5
Average stars matched: 37772.5 (96.2884 %)
Memory usage VmPeak: 145312 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Feb 27 02:34:48 CST 2026
Host name: tau
############################################################
######## Processing parameters ########
AAVSO_COMMENT_STRING= NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
ASTCHECK_ASTEROID_SEARCH_RADIUS_ARCSEC=
BAD_REGION_FILE= /var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst
CAMERA_SETTINGS= TTUQ2b1x1
CHECK_POINTING_ACCURACY= yes
DARK_FRAMES_DIR=
EXCLUSION_LIST= ../exclusion_list_TTUQ2.txt
FILTER_BAD_IMG__MAX_APERTURE_STAR_SIZE_PIX= 12.5
FILTER_BAD_IMG__MAX_ELONGATION_AminusB_PIX= 0.55
FILTER_BAD_IMG__MIN_APERTURE_STAR_SIZE_PIX= 2.0
FILTER_BRIGHT_MAG_CUTOFF_TRANSIENT_SEARCH= -5
FILTER_FAINT_MAG_CUTOFF_TRANSIENT_SEARCH= 14.5
FLAT_FIELD_FILE=
FRAME_EDGE_OFFSET_PIX= 100
GAIA_BAND_FOR_CATALOGED_SOURCE_CHECK=
MAX_NEW_TO_REF_MEAN_IMG_VALUE_RATIO= 100
MAX_NEW_IMG_MEAN_VALUE= 25000
MAX_SD_RATIO_OF_SECOND_EPOCH_IMGS= 0.18
MAX_SD_RATIO_OF_SECOND_EPOCH_IMGS_SOFT_LIMIT= 0.12
MPC_CODE= 500
NMW_CALIBRATION= /var/www/nmw_calibration
NUMBER_OF_DETECTED_TRANSIENTS_BEFORE_FILTERING_HARD_LIMIT= 3000
NUMBER_OF_DETECTED_TRANSIENTS_BEFORE_FILTERING_SOFT_LIMIT= 2000
OMP_NUM_THREADS=
ONLINE_MPCHECKER_BUTTON_ASTEROID_SEARCH_RADIUS_ARCMIN=
PHOTOMETRIC_CALIBRATION=
REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES= yes
SEXTRACTOR_CONFIG_BRIGHTSTARPASS= default.sex.telephoto_lens_onlybrightstars_v1
SEXTRACTOR_CONFIG_FILES= default.sex.telephoto_lens_onlybrightstars_v1 default.sex.telephoto_lens_vSTL
STARMATCH_RADIUS_PIX= 3.5
SYSREM_ITERATIONS= 0
TELESCOP=
TELESCOP_NAME_KNOWN_TO_VaST_FOR_FOV_DETERMINATION=
UCAC5_PLATESOLVE_ITERATIONS= 2
FPACK_FULLY_CALIBRATED_IMAGE= no
#######################################
HOSTNAME= tau
USER=
HOME=
#######################################
SExtractor catalog cache: enabled, directory /data_ssd/NMW-TexasTech/vast_sextractor_cache
Reference image directory is set to /data_ssd/NMW-TexasTech/reference_imgs
VIZIER_SITE=vizier.cds.unistra.fr
GAIA_DR2_CLIENT=vizquery (lib/vizquery -> VizieR vizier.cds.unistra.fr)
INFO: MAKE_PNG_PLOTS is set to yes
FITS_FILE_EXT=fits
CALIBRATION_STATUS_PREFIX=
Fields in the data directory:
Hya-09-Q2b1x1
#######################################
########### Starting Hya-09-Q2b1x1 ###########
Processing Hya-09-Q2b1x1
server tau has sufficient free disk space available: 741550 MB at /data_ssd/NMW-TexasTech/workdir
server tau has sufficient free disk space available: 741550 MB at .
Checking input images (2 new)
REFERENCE_EPOCH__FIRST_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
REFERENCE_EPOCH__SECOND_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
Small preview (one of the new images):
Large previews of the second-epoch (new) images:
MAKE_PNG_PLOTS=yes
renamed 'Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.png' -> 'transient_report/Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits_preview.png'
Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits
renamed 'Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.png' -> 'transient_report/Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits_preview.png'
Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits
Read-check the input FITS images... read-check OK
Blank image check the input FITS images... blank-image-check OK
Read date check the input FITS images... read-date-check OK
Mean value check the input FITS images... OK, at least two new images have mean values below the threshold.
----------------------------------------------
INFO: REFERENCE_EPOCH__FIRST_IMAGE_MEAN_VALUE= 1279.4931
INFO: REFERENCE_EPOCH__FIRST_IMAGE_SD= 607.8106
INFO: SECOND_EPOCH__FIRST_IMAGE_MEAN_VALUE= 3043.2312
INFO: SECOND_EPOCH__FIRST_IMAGE_SD= 826.2678
INFO: SECOND_EPOCH__SECOND_IMAGE_MEAN_VALUE= 3036.7888
INFO: SECOND_EPOCH__SECOND_IMAGE_SD= 825.4606
----------------------------------------------
INFO: ref_to_second_epoch_img_mean_ratio= 2.37847
INFO: SECOND_EPOCH__SD_ratio= 0.001
----------------------------------------------
Calibration settings: DARK_FRAMES_DIR= FLAT_FIELD_FILE=
try_to_calibrate_the_input_frame(): DARK_FRAMES_DIR is not set - not attempting to dark-subtract the input frames
try_to_calibrate_the_input_frame(): DARK_FRAMES_DIR is not set - not attempting to dark-subtract the input frames
after the calibration attempt:
SECOND_EPOCH__FIRST_IMAGE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits
SECOND_EPOCH__SECOND_IMAGE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits
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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits
SExtractor catalog cache: saved Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat to cache
SExtractor catalog cache: saved Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461098.72132431
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-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits exists and is non-empty
Saving wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits to local_wcs_cache/
'wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits' -> 'local_wcs_cache/wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits'
wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits exists and is non-empty
Saving wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits to local_wcs_cache/
'wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits' -> 'local_wcs_cache/wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits'
wcs_Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits exists and is non-empty
Saving wcs_Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits to local_wcs_cache/
'wcs_Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits' -> 'local_wcs_cache/wcs_Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits'
wcs_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits exists and is non-empty
Saving wcs_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits to local_wcs_cache/
'wcs_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits' -> 'local_wcs_cache/wcs_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 10:39:59.375 -17:59:54.09
Second-epoch image center 10:39:52.768 -17:57:08.42
Angular distance between the image centers 0.05 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 10:39:59.375 -17:59:54.09
Second-epoch image center 10:39:51.185 -17:57:26.35
Angular distance between the image centers 0.05 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 10:39:52.768 -17:57:08.42
Second-epoch second image center 10:39:51.185 -17:57:26.35
Angular distance between the image centers 0.00801 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits &> /tmp/tmp.2ypf9Swqam
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits &> /tmp/tmp.AUvNAZzq3O
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits &> /tmp/tmp.3TF8xHemEy
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits &> /tmp/tmp.5dyyWw90tj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits and wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits and wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat
Found non-empty wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits and wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat
The reference image (wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits) and catalog (wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat) found
'wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat' -> 'wcsmag.cat'
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 5250 out of 7725 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.887548
a=0.000000 b=1.000000 c=22.887548
From vast_summary.log: estimated ref. image limiting mag.: -7.97
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.92
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.92
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
2.1 pix Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
2.4 pix Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits
2.4 pix Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits
Limiting magnitude estimates:
14.9 mag. Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
14.9 mag. Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
14.3 mag. Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits
14.3 mag. Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 11.4 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.2ypf9Swqam (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-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.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_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.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-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits' -> 'wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
WCS_IMAGE_NAME=wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
WCS-calibrated image found: wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
Checking if the catalog wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat corresponding to the image wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits alredy exist and is non-empty...
Catalog wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat corresponding to the image wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
WCS catalog name: wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=533, passed=7725
Got 7725 stars (including 7185 good ones) from the SExtractor catalog wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat
util/solve_plate_with_UCAC5 got 7725 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.26"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.26"
Estimated accuracy of the plate solution: 0.24"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits -region wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.AUvNAZzq3O (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-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.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_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.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-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits' -> 'wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
WCS_IMAGE_NAME=wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
WCS-calibrated image found: wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
Checking if the catalog wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat corresponding to the image wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits alredy exist and is non-empty...
Catalog wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat corresponding to the image wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
WCS catalog name: wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=531, passed=7630
Got 7630 stars (including 7093 good ones) from the SExtractor catalog wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat
util/solve_plate_with_UCAC5 got 7630 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.27"
Estimated accuracy of the plate solution: 0.24"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits -region wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.3TF8xHemEy (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits
WCS_IMAGE_NAME=wcs_Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits
WCS-calibrated image found: wcs_Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits
Checking if the catalog wcs_Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits.cat corresponding to the image wcs_Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits alredy exist and is non-empty...
Catalog wcs_Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits.cat corresponding to the image wcs_Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits
WCS catalog name: wcs_Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=552, passed=4894
Got 4894 stars (including 4336 good ones) from the SExtractor catalog wcs_Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits.cat
util/solve_plate_with_UCAC5 got 4894 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.39"
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits -region wcs_Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.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.5dyyWw90tj (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits
WCS_IMAGE_NAME=wcs_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits
WCS-calibrated image found: wcs_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits
Checking if the catalog wcs_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits.cat corresponding to the image wcs_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits alredy exist and is non-empty...
Catalog wcs_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits.cat corresponding to the image wcs_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits
WCS catalog name: wcs_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=537, passed=4898
Got 4898 stars (including 4353 good ones) from the SExtractor catalog wcs_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits.cat
util/solve_plate_with_UCAC5 got 4898 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
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 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.37"
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits -region wcs_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.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
WARNING: no fully-calibrated images to save!
Preparing the HTML report for the field Hya-09-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20382.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20383.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20385.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
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 20382_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060
The candidate 20382_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 10:56:51.90 -20:26:01.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.12, MAG_FAINT_SEARCH_LIMIT=12.10)GAIADR2_OUTPUT=# 2.324 3552237403208380800 164.21693215298 -20.43392421023 12.0149 10.2224 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.324#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20383_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060
The candidate 20383_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 10:27:47.40 -19:52:51.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.46, MAG_FAINT_SEARCH_LIMIT=12.44)GAIADR2_OUTPUT=# 0.398 5668493855827181696 156.94753223728 -19.88102295467 11.4918 11.0678 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.398#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20385_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060
The candidate 20385_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 10:39:02.29 -18:16:56.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.78, MAG_FAINT_SEARCH_LIMIT=12.76)GAIADR2_OUTPUT=# 0.444 3555364547420624000 159.75965519569 -18.28253196832 11.9407 11.3610 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.444#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Hya-09-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 ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits
SExtractor catalog cache: saved Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat to cache
SExtractor catalog cache: saved Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
Creating symlink local_wcs_cache/wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
Creating symlink local_wcs_cache/wcs_Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits
Creating symlink local_wcs_cache/wcs_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits exists and is non-empty
wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits exists and is non-empty
wcs_Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits exists and is non-empty
wcs_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 10:39:59.375 -17:59:54.09
Second-epoch image center 10:39:52.768 -17:57:08.42
Angular distance between the image centers 0.05 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 10:39:59.375 -17:59:54.09
Second-epoch image center 10:39:51.185 -17:57:26.35
Angular distance between the image centers 0.05 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 10:39:52.768 -17:57:08.42
Second-epoch second image center 10:39:51.185 -17:57:26.35
Angular distance between the image centers 0.00801 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits &> /tmp/tmp.wJd3NmeW4s
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits &> /tmp/tmp.duWkFfwkc1
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits &> /tmp/tmp.cyH3eS0OoO
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits &> /tmp/tmp.bH0RoPUJQn
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits and wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits and wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat
Found non-empty wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits and wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat
The reference image (wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits) and catalog (wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat) found
'wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat' -> 'wcsmag.cat'
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 5627 out of 46060 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.755505
a=0.000000 b=1.000000 c=22.755505
From vast_summary.log: estimated ref. image limiting mag.: -7.73
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.03
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.03
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 42 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
2.0 pix Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
2.2 pix Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits
2.2 pix Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits
Limiting magnitude estimates:
15.0 mag. Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
15.0 mag. Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
14.4 mag. Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits
14.4 mag. Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 13.8 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.wJd3NmeW4s (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-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.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_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.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-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits' -> 'wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
WCS_IMAGE_NAME=wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
WCS-calibrated image found: wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
Checking if the catalog wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat corresponding to the image wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits alredy exist and is non-empty...
Catalog wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat corresponding to the image wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
WCS catalog name: wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=1888, passed=46057
Got 46057 stars (including 44088 good ones) from the SExtractor catalog wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat
util/solve_plate_with_UCAC5 got 46057 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.28"
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits -region wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.duWkFfwkc1 (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-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.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_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.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-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits' -> 'wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
WCS_IMAGE_NAME=wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
WCS-calibrated image found: wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
Checking if the catalog wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat corresponding to the image wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits alredy exist and is non-empty...
Catalog wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat corresponding to the image wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
WCS catalog name: wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=1954, passed=46667
Got 46667 stars (including 44657 good ones) from the SExtractor catalog wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat
util/solve_plate_with_UCAC5 got 46667 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.29"
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits -region wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.cyH3eS0OoO (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits
WCS_IMAGE_NAME=wcs_Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits
WCS-calibrated image found: wcs_Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits
Checking if the catalog wcs_Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits.cat corresponding to the image wcs_Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits alredy exist and is non-empty...
Catalog wcs_Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits.cat corresponding to the image wcs_Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits
WCS catalog name: wcs_Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=1503, passed=32601
Got 32601 stars (including 31041 good ones) from the SExtractor catalog wcs_Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits.cat
util/solve_plate_with_UCAC5 got 32601 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.38"
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits -region wcs_Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-09-Q2b1x1_2026-02-26_23-18-32_20.00sec_-14.90C_LIGHT_0059.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.bH0RoPUJQn (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits
WCS_IMAGE_NAME=wcs_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits
WCS-calibrated image found: wcs_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits
Checking if the catalog wcs_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits.cat corresponding to the image wcs_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits alredy exist and is non-empty...
Catalog wcs_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits.cat corresponding to the image wcs_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits
WCS catalog name: wcs_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=1509, passed=32654
Got 32654 stars (including 31093 good ones) from the SExtractor catalog wcs_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits.cat
util/solve_plate_with_UCAC5 got 32654 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
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 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.38"
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-09-Q2b1x1_234344_TTUQ2b1x1_14006_25JvmK7I/Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits -region wcs_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060.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
WARNING: no fully-calibrated images to save!
Preparing the HTML report for the field Hya-09-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out30763.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53702.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53704.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53706.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53708.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53719.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53720.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53723.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53724.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53725.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53726.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53727.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53729.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53730.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53731.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53732.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53765.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53851.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53939.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53955.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53970.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53993.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54002.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54023.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54071.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54191.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54199.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54276.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54423.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54472.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54478.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54512.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54550.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out15170.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33877.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 53702_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060
The candidate 53702_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 10:08:48.49 -19:35:18.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 0.777 5669264819636469504 152.20192504077 -19.58863013702 13.5530 13.0403 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.777#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53704_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060
The candidate 53704_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 10:08:20.66 -20:47:50.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 0.431 5667446914598984448 152.08597817996 -20.79740177089 14.1222 13.6399 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.431#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53705_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060
The candidate 53705_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
Rejecting candidate due to large distance (16.4") between the two second-epoch detections
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Considering the candidate 53706_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060
The candidate 53706_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 11:05:17.12 -21:03:46.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.37, MAG_FAINT_SEARCH_LIMIT=15.35)GAIADR2_OUTPUT=# 0.829 3551252446948207488 166.32112880318 -21.06301753822 13.8226 13.2197 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.829#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53708_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060
The candidate 53708_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 10:56:19.91 -18:00:24.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)GAIADR2_OUTPUT=# 0.720 3555800576796132992 164.08293722527 -18.00646753975 14.5466 13.9581 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.720#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53719_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060
The candidate 53719_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 11:03:34.44 -13:03:57.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)
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Considering the candidate 53720_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060
The candidate 53720_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 10:13:51.98 -19:57:24.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)
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Considering the candidate 53721_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060
The candidate 53721_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 10:48:02.98 -13:25:29.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53723_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060
The candidate 53723_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 10:47:21.47 -19:58:04.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 0.737 3554011430860139008 161.83925413496 -19.96804338848 13.7532 13.1749 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.737#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53724_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060
The candidate 53724_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 10:23:47.85 -15:04:37.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 4.897 3752144383961960960 155.95033378572 -15.07810776417 13.4489 12.7866 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.897#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53725_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060
The candidate 53725_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 10:13:50.37 -13:25:09.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 2.256 3753169648490505728 153.46034128633 -13.41973797103 12.4633 11.9709 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.256#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53726_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060
The candidate 53726_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 10:51:12.94 -20:21:17.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 0.649 3551018766368339584 162.80398810941 -20.35505627322 13.2272 12.6040 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.649#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53727_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060
The candidate 53727_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 10:57:39.50 -12:57:41.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 0.403 3756585968557248768 164.41468655492 -12.96153415880 13.0006 12.5305 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.403#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53729_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060
The candidate 53729_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 11:00:53.29 -19:35:34.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 0.626 3552388238163811968 165.22196346152 -19.59310181283 13.0842 12.5770 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.626#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53730_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060
The candidate 53730_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 10:51:59.81 -13:06:09.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 1.147 3756429902330424704 162.99904332528 -13.10239154732 12.5083 11.7766 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.147#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53731_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060
The candidate 53731_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 10:18:16.90 -13:37:46.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)
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Considering the candidate 53732_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060
The candidate 53732_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 10:59:13.22 -17:32:28.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 0.804 3556211686769923968 164.80516589251 -17.54092982409 12.5043 12.0293 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.804#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53765_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060
The candidate 53765_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 10:56:51.88 -20:26:01.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.38, MAG_FAINT_SEARCH_LIMIT=12.36)GAIADR2_OUTPUT=# 2.603 3552237403208380800 164.21693215298 -20.43392421023 12.0149 10.2224 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.603#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53851_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060
The candidate 53851_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 11:01:25.25 -16:54:17.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 0.635 3556356135110207232 165.35504449653 -16.90475262476 12.5050 12.0542 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.635#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53878_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060
The candidate 53878_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 11:11:31.86 -22:50:14.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 53939_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060
The candidate 53939_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 10:56:40.91 -20:39:56.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.00, MAG_FAINT_SEARCH_LIMIT=13.98)GAIADR2_OUTPUT=# 0.823 3550728937678924032 164.17022974490 -20.66580278947 13.0745 12.4992 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.823#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53955_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060
The candidate 53955_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 10:11:20.80 -18:55:35.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 1.962 5669405179167736064 152.83702954215 -18.92618784652 12.7388 12.3482 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.962#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53970_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060
The candidate 53970_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 10:34:00.61 -17:47:34.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 2.278 3747629793513719168 158.50304201542 -17.79252803560 13.2459 12.7383 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.278#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53993_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060
The candidate 53993_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 10:52:59.06 -20:37:19.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 2.011 3550949943812507520 163.24549956897 -20.62196688772 13.4524 13.0078 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.011#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54002_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060
The candidate 54002_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 10:45:39.78 -21:10:09.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 0.474 3550488526885505536 161.41588569121 -21.16939729771 13.4245 12.8930 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.474#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54023_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060
The candidate 54023_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 10:47:36.62 -15:06:19.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 2.974 3749864585257273088 161.90193127847 -15.10499294941 13.4847 12.9357 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.974#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54071_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060
The candidate 54071_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 11:04:27.65 -21:18:32.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 0.662 3551148199502129920 166.11511996213 -21.30924767638 13.2117 12.7236 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.662#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54075_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060
The candidate 54075_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 11:00:08.16 -14:03:27.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 54191_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060
The candidate 54191_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 11:08:56.60 -19:00:57.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 3.907 3552105496173004416 167.23468591987 -19.01585619096 13.8923 13.4491 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.907#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54199_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060
The candidate 54199_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 10:57:15.37 -17:45:54.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 2.254 3556227977581543424 164.31362009130 -17.76454750344 13.7847 12.8657 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.254#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54276_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060
The candidate 54276_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 10:41:40.70 -20:03:48.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 0.800 3553821352786877184 160.41964241327 -20.06360408765 14.3884 13.7987 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.800#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54309_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060
The candidate 54309_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 10:40:50.16 -13:26:22.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54423_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060
The candidate 54423_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 10:56:26.91 -20:21:10.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 0.571 3552285953518653312 164.11218389896 -20.35265690972 14.3235 13.8035 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.571#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54472_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060
The candidate 54472_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 11:02:50.86 -17:16:22.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.32, MAG_FAINT_SEARCH_LIMIT=15.30)GAIADR2_OUTPUT=# 0.537 3553327775145483008 165.71189720278 -17.27303698995 14.5374 13.9743 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.537#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54478_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060
The candidate 54478_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 11:08:11.46 -15:28:12.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.44, MAG_FAINT_SEARCH_LIMIT=15.42)GAIADR2_OUTPUT=# 0.844 3562557213187781760 167.04798845650 -15.47003657231 14.3937 13.8394 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 54494_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060
The candidate 54494_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 54512_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060
The candidate 54512_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 11:01:22.05 -18:57:02.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 2.387 3552490978077962240 165.34119773808 -18.95046792614 14.6487 14.1558 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.387#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54550_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060
The candidate 54550_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 10:59:53.76 -13:14:07.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 1.028 3564402846534320640 164.97428934599 -13.23540847988 14.3562 13.8572 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.028#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 33877_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 33877_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 30763_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060
The candidate 30763_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks
**** FOUND 10:17:49.47 -13:06:02.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 2.061 3753533445104814592 154.45554409930 -13.10069115178 12.5373 12.0217 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.061#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 15170_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060
Preparing report for the candidate 15170_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060
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Considering the candidate 19830_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060
The candidate 19830_Hya-09-Q2b1x1_2026-02-26_23-19-17_20.00sec_-15.00C_LIGHT_0060 did not pass the final checks