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 J103933-2550.6,2461098.7141,13.09,0.05,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 J103933-2550.6 20260227.2141 13.09CV 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
######## 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-10-Q2b1x1
#######################################
########### Starting Hya-10-Q2b1x1 ###########
Processing Hya-10-Q2b1x1
server tau has sufficient free disk space available: 711854 MB at /data_ssd/NMW-TexasTech/workdir
server tau has sufficient free disk space available: 711854 MB at .
Checking input images (2 new)
REFERENCE_EPOCH__FIRST_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
REFERENCE_EPOCH__SECOND_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
Small preview (one of the new images): 
Large previews of the second-epoch (new) images:
MAKE_PNG_PLOTS=yes
renamed 'Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.png' -> 'transient_report/Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits_preview.png'
Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits

renamed 'Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.png' -> 'transient_report/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits_preview.png'
Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.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= 1679.5694
INFO: REFERENCE_EPOCH__FIRST_IMAGE_SD= 620.4944
INFO: SECOND_EPOCH__FIRST_IMAGE_MEAN_VALUE= 3993.7967
INFO: SECOND_EPOCH__FIRST_IMAGE_SD= 1023.9124
INFO: SECOND_EPOCH__SECOND_IMAGE_MEAN_VALUE= 3981.9950
INFO: SECOND_EPOCH__SECOND_IMAGE_SD= 1021.6774
----------------------------------------------
INFO: ref_to_second_epoch_img_mean_ratio= 2.37787
INFO: SECOND_EPOCH__SD_ratio= 0.002
----------------------------------------------
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-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits
SECOND_EPOCH__SECOND_IMAGE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.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-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits
SExtractor catalog cache: saved Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits.cat to cache
SExtractor catalog cache: saved Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.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-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.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: 2461098.71384287
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-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits exists and is non-empty
Saving wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits to local_wcs_cache/
'wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits' -> 'local_wcs_cache/wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits'
wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits exists and is non-empty
Saving wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits to local_wcs_cache/
'wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits' -> 'local_wcs_cache/wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits'
wcs_Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits exists and is non-empty
Saving wcs_Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits to local_wcs_cache/
'wcs_Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits' -> 'local_wcs_cache/wcs_Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits'
wcs_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits exists and is non-empty
Saving wcs_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits to local_wcs_cache/
'wcs_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits' -> 'local_wcs_cache/wcs_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.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 10:33:37.466 -25:59:59.61
Second-epoch image center 10:33:38.279 -25:58:22.81
Angular distance between the image centers 0.03 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 10:33:37.466 -25:59:59.61
Second-epoch image center 10:33:40.229 -25:58:02.37
Angular distance between the image centers 0.03 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 10:33:38.279 -25:58:22.81
Second-epoch second image center 10:33:40.229 -25:58:02.37
Angular distance between the image centers 0.00925 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-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits &> /tmp/tmp.LsoxpqhzGg
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits &> /tmp/tmp.rlS1JVtb09
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits &> /tmp/tmp.FqfBiWxN55
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits &> /tmp/tmp.KhfifbYbYB
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.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-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits and wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.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-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits and wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits.cat
Found non-empty wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits and wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits.cat
The reference image (wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits) and catalog (wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits.cat) found
'wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.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 6213 out of 8052 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.818359
a=0.000000 b=1.000000 c=22.818359
From vast_summary.log: estimated ref. image limiting mag.: -8.11
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.71
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.71
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
2.0 pix Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
2.4 pix Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits
2.4 pix Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits
Limiting magnitude estimates:
14.7 mag. Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
14.7 mag. Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
14.0 mag. Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits
14.0 mag. Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 11.3 (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.LsoxpqhzGg (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-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.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-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.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-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.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-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits' -> 'wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
WCS_IMAGE_NAME=wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
WCS-calibrated image found: wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
Checking if the catalog wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits.cat corresponding to the image wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits alredy exist and is non-empty...
Catalog wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits.cat corresponding to the image wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
WCS catalog name: wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=581, passed=8052
Got 8052 stars (including 7465 good ones) from the SExtractor catalog wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits.cat
util/solve_plate_with_UCAC5 got 8052 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.27"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits -region wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.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.rlS1JVtb09 (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-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.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-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.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-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.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-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits' -> 'wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
WCS_IMAGE_NAME=wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
WCS-calibrated image found: wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
Checking if the catalog wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits.cat corresponding to the image wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits alredy exist and is non-empty...
Catalog wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits.cat corresponding to the image wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
WCS catalog name: wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=565, passed=8068
Got 8068 stars (including 7487 good ones) from the SExtractor catalog wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits.cat
util/solve_plate_with_UCAC5 got 8068 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 961 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 960 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: 0.27"
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-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits -region wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.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.FqfBiWxN55 (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-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.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-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits
WCS_IMAGE_NAME=wcs_Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits
WCS-calibrated image found: wcs_Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits
Checking if the catalog wcs_Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits.cat corresponding to the image wcs_Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits alredy exist and is non-empty...
Catalog wcs_Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits.cat corresponding to the image wcs_Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.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-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits
WCS catalog name: wcs_Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=541, passed=5093
Got 5093 stars (including 4552 good ones) from the SExtractor catalog wcs_Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits.cat
util/solve_plate_with_UCAC5 got 5093 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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 961 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: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.42"
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits -region wcs_Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.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.KhfifbYbYB (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-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.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-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits
WCS_IMAGE_NAME=wcs_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits
WCS-calibrated image found: wcs_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits
Checking if the catalog wcs_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits.cat corresponding to the image wcs_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits alredy exist and is non-empty...
Catalog wcs_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits.cat corresponding to the image wcs_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.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-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits
WCS catalog name: wcs_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=522, passed=5128
Got 5128 stars (including 4601 good ones) from the SExtractor catalog wcs_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits.cat
util/solve_plate_with_UCAC5 got 5128 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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 963 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 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.40"
Estimated accuracy of the plate solution: 0.40"
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-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits -region wcs_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.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-10-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20438.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20442.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: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20438_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048
The candidate 20438_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
| Discovery image 2 | 2026 02 27.21439 | 2461098.71439 | 11.24 | 10:36:24.71 -24:34:44.3 | 5159 4035 | /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits |
**** FOUND 10:36:24.71 -24:34:44.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.24, MAG_FAINT_SEARCH_LIMIT=12.22)GAIADR2_OUTPUT=# 1.507 5470983187651504512 159.10324920153 -24.57924115055 11.5596 11.1168 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.507#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20442_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048
The candidate 20442_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
| Discovery image 2 | 2026 02 27.21439 | 2461098.71439 | 11.41 | 10:11:16.54 -27:14:12.7 | 1779 2334 | /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits |
**** FOUND 10:11:16.53 -27:14:12.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.50, MAG_FAINT_SEARCH_LIMIT=12.48)GAIADR2_OUTPUT=# 0.257 5466019545487196800 152.81895449681 -27.23682336390 11.4376 11.0770 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.257#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: 1s
Prepared the HTML report for the field Hya-10-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-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits
SExtractor catalog cache: saved Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits.cat to cache
SExtractor catalog cache: saved Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.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-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
Creating symlink local_wcs_cache/wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
Creating symlink local_wcs_cache/wcs_Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits
Creating symlink local_wcs_cache/wcs_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.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-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits exists and is non-empty
wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits exists and is non-empty
wcs_Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits exists and is non-empty
wcs_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.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 10:33:37.466 -25:59:59.61
Second-epoch image center 10:33:38.279 -25:58:22.81
Angular distance between the image centers 0.03 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 10:33:37.466 -25:59:59.61
Second-epoch image center 10:33:40.229 -25:58:02.37
Angular distance between the image centers 0.03 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 10:33:38.279 -25:58:22.81
Second-epoch second image center 10:33:40.229 -25:58:02.37
Angular distance between the image centers 0.00925 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-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits &> /tmp/tmp.1O7uKucUef
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits &> /tmp/tmp.tLDz1reelu
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits &> /tmp/tmp.tF7q18mbEs
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits &> /tmp/tmp.szxT7oCkny
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.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-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits and wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.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-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits and wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits.cat
Found non-empty wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits and wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits.cat
The reference image (wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits) and catalog (wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits.cat) found
'wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.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 7312 out of 56496 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.651562
a=0.000000 b=1.000000 c=22.651562
From vast_summary.log: estimated ref. image limiting mag.: -7.81
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.84
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.84
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 31 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
1.9 pix Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
2.2 pix Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits
2.2 pix Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits
Limiting magnitude estimates:
14.8 mag. Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
14.8 mag. Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
14.2 mag. Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits
14.1 mag. Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 13.6 (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.1O7uKucUef (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-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.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-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.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-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.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-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits' -> 'wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
WCS_IMAGE_NAME=wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
WCS-calibrated image found: wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
Checking if the catalog wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits.cat corresponding to the image wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits alredy exist and is non-empty...
Catalog wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits.cat corresponding to the image wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits
WCS catalog name: wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=2594, passed=56489
Got 56489 stars (including 53792 good ones) from the SExtractor catalog wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits.cat
util/solve_plate_with_UCAC5 got 56489 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.30"
Estimated accuracy of the plate solution: 0.30"
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-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits -region wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-10-Q2b1x1_2026-01-21_02-59-12_20.00sec_-15.00C_LIGHT_0426.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.tLDz1reelu (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-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.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-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.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-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.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-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits' -> 'wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
WCS_IMAGE_NAME=wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
WCS-calibrated image found: wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
Checking if the catalog wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits.cat corresponding to the image wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits alredy exist and is non-empty...
Catalog wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits.cat corresponding to the image wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits
WCS catalog name: wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=2585, passed=55964
Got 55964 stars (including 53278 good ones) from the SExtractor catalog wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits.cat
util/solve_plate_with_UCAC5 got 55964 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.30"
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits -region wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-10-Q2b1x1_2026-01-21_03-00-16_20.00sec_-15.00C_LIGHT_0427.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.tF7q18mbEs (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-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.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-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits
WCS_IMAGE_NAME=wcs_Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits
WCS-calibrated image found: wcs_Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits
Checking if the catalog wcs_Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits.cat corresponding to the image wcs_Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits alredy exist and is non-empty...
Catalog wcs_Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits.cat corresponding to the image wcs_Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.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-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits
WCS catalog name: wcs_Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=1718, passed=36367
Got 36367 stars (including 34592 good ones) from the SExtractor catalog wcs_Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits.cat
util/solve_plate_with_UCAC5 got 36367 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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 963 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: 0.41"
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: 0.41"
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits -region wcs_Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-10-Q2b1x1_2026-02-26_23-07-46_20.00sec_-14.90C_LIGHT_0047.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.szxT7oCkny (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-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.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-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits
WCS_IMAGE_NAME=wcs_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits
WCS-calibrated image found: wcs_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits
Checking if the catalog wcs_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits.cat corresponding to the image wcs_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits alredy exist and is non-empty...
Catalog wcs_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits.cat corresponding to the image wcs_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.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-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits
WCS catalog name: wcs_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=1673, passed=36190
Got 36190 stars (including 34472 good ones) from the SExtractor catalog wcs_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits.cat
util/solve_plate_with_UCAC5 got 36190 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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 964 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: 0.39"
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: 0.39"
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits -region wcs_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.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-10-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out70756.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70759.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70760.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70761.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70764.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70778.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70780.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70786.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70788.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70789.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70794.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70944.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71005.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71046.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71065.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71153.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71191.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71231.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71366.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71432.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71458.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71551.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out30470.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 70756_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048
The candidate 70756_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
| Discovery image 2 | 2026 02 27.21439 | 2461098.71439 | 13.96 | 09:58:17.86 -30:16:47.9 | 0145 0355 | /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits |
**** FOUND 09:58:17.86 -30:16:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 1.387 5463735447520190848 149.57461445988 -30.28012306962 13.2856 12.6415 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.387#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70759_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048
The candidate 70759_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
| Discovery image 2 | 2026 02 27.21439 | 2461098.71439 | 13.86 | 10:42:49.71 -25:23:43.9 | 6036 3540 | /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits |
**** FOUND 10:42:49.73 -25:23:44.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 1.077 5470086295400940288 160.70747873056 -25.39543817212 14.0209 13.2731 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.077#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70760_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048
The candidate 70760_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
| Discovery image 2 | 2026 02 27.21439 | 2461098.71439 | 13.94 | 11:01:42.13 -24:49:03.5 | 8646 3825 | /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits |
**** FOUND 11:01:42.11 -24:49:04.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 1.220 3536609632126860288 165.42582294738 -24.81787183102 13.8796 13.3330 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.220#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70761_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048
The candidate 70761_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
| Discovery image 2 | 2026 02 27.21439 | 2461098.71439 | 14.01 | 10:02:23.10 -30:04:49.9 | 0683 0523 | /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits |
**** FOUND 10:02:22.94 -30:04:50.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.97, MAG_FAINT_SEARCH_LIMIT=14.95)GAIADR2_OUTPUT=# 3.162 5463659512498092672 150.59659821402 -30.08068194113 13.6770 13.2582 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.162#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70764_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048
The candidate 70764_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
| Discovery image 2 | 2026 02 27.21439 | 2461098.71439 | 14.12 | 11:06:13.90 -23:38:36.6 | 9319 4512 | /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits |
**** FOUND 11:06:13.89 -23:38:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 2.893 3537175983694126976 166.55717582528 -23.64409632908 13.7162 13.1955 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.893#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70770_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048
The candidate 70770_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
| Discovery image 2 | 2026 02 27.21439 | 2461098.71439 | 13.21 | 10:03:05.38 -22:25:01.6 | 0467 5200 | /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits |
**** FOUND 10:03:05.37 -22:25:02.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70778_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048
The candidate 70778_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
| Discovery image 2 | 2026 02 27.21439 | 2461098.71439 | 13.59 | 11:05:09.57 -22:03:18.9 | 9221 5490 | /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits |
**** FOUND 11:05:09.59 -22:03:18.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 0.949 3539063909581973120 166.29017576960 -22.05536420624 13.2463 12.9079 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.949#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70779_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048
The candidate 70779_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
| Discovery image 2 | 2026 02 27.21439 | 2461098.71439 | 13.18 | 10:45:39.75 -21:10:11.9 | 6463 6099 | /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits |
**** FOUND 10:45:39.78 -21:10:11.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70780_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048
The candidate 70780_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
| Discovery image 2 | 2026 02 27.21439 | 2461098.71439 | 13.28 | 11:07:47.17 -30:34:34.4 | 9299 0270 | /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits |
**** FOUND 11:07:47.39 -30:34:34.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 1.572 5452268675113581440 166.94696254881 -30.57604691495 12.1220 11.7373 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.572#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70786_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048
The candidate 70786_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
| Discovery image 2 | 2026 02 27.21439 | 2461098.71439 | 12.95 | 10:07:05.36 -27:50:40.0 | 1232 1932 | /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits |
**** FOUND 10:07:05.40 -27:50:40.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 1.433 5465650384458404096 151.77292682738 -27.84457088346 13.1692 12.7289 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.433#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70788_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048
The candidate 70788_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
| Discovery image 2 | 2026 02 27.21439 | 2461098.71439 | 12.86 | 10:12:37.16 -30:46:09.1 | 2062 0196 | /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits |
**** FOUND 10:12:37.20 -30:46:08.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 0.814 5461820579300828416 153.15503670561 -30.76891488010 12.7837 12.1984 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.814#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70789_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048
The candidate 70789_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
| Discovery image 2 | 2026 02 27.21439 | 2461098.71439 | 12.99 | 10:49:09.63 -22:11:14.0 | 6946 5473 | /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits |
**** FOUND 10:49:09.67 -22:11:14.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 1.774 3550135136975993856 162.28991025512 -22.18696204240 13.1389 12.5257 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.774#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70791_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048
The candidate 70791_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
| Discovery image 2 | 2026 02 27.21439 | 2461098.71439 | 12.61 | 10:00:22.51 -24:55:21.1 | 0191 3647 | /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits |
**** FOUND 10:00:22.45 -24:55:20.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70794_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048
The candidate 70794_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
| Discovery image 2 | 2026 02 27.21439 | 2461098.71439 | 12.51 | 10:43:34.40 -29:59:56.6 | 6109 0754 | /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits |
**** FOUND 10:43:34.38 -29:59:57.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 0.155 5454786243206469376 160.89323116568 -29.99940084798 12.2236 11.2962 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.155#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70944_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048
The candidate 70944_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
| Discovery image 2 | 2026 02 27.21439 | 2461098.71439 | 12.73 | 11:01:25.43 -28:10:11.9 | 8516 1790 | /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits |
**** FOUND 11:01:25.47 -28:10:11.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 1.284 5453711990283449088 165.35579617711 -28.17015210824 12.5599 11.9829 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.284#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71005_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048
The candidate 71005_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
| Discovery image 2 | 2026 02 27.21439 | 2461098.71439 | 12.83 | 11:00:38.05 -27:29:05.8 | 8427 2212 | /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits |
**** FOUND 11:00:38.04 -27:29:06.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 1.350 5456845632782590464 165.15808437604 -27.48495918059 12.7549 12.0983 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.350#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71046_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048
The candidate 71046_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
| Discovery image 2 | 2026 02 27.21439 | 2461098.71439 | 13.22 | 10:49:45.45 -28:55:09.5 | 6937 1394 | /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits |
**** FOUND 10:49:45.36 -28:55:08.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)GAIADR2_OUTPUT=# 1.196 5456419056630646528 162.43934205336 -28.91903318939 13.1939 12.5859 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.196#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71065_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048
The candidate 71065_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
| Discovery image 2 | 2026 02 27.21439 | 2461098.71439 | 13.13 | 10:53:18.99 -30:05:56.3 | 7391 0662 | /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits |
**** FOUND 10:53:19.02 -30:05:56.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 0.198 5453103513676843136 163.32929541433 -30.09901709757 12.8595 12.2525 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.198#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71090_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048
The candidate 71090_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
| Discovery image 2 | 2026 02 27.21439 | 2461098.71439 | 13.16 | 10:29:25.05 -29:38:11.1 | 4248 0969 | /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits |
**** FOUND 10:29:25.00 -29:38:09.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 71153_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048
The candidate 71153_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
| Discovery image 2 | 2026 02 27.21439 | 2461098.71439 | 13.42 | 10:58:17.61 -25:00:40.6 | 8168 3726 | /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits |
**** FOUND 10:58:17.58 -25:00:39.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 3.768 3536564827028011264 164.57221411926 -25.01154618058 13.4872 12.9591 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.768#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71191_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048
The candidate 71191_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
| Discovery image 2 | 2026 02 27.21439 | 2461098.71439 | 13.52 | 11:01:24.16 -29:36:00.8 | 8476 0919 | /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits |
**** FOUND 11:01:24.11 -29:36:01.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 1.184 5452994627665709056 165.35027665262 -29.60062167698 13.1342 12.4521 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.184#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71231_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048
The candidate 71231_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
| Discovery image 2 | 2026 02 27.21439 | 2461098.71439 | 13.71 | 10:54:58.31 -24:19:10.1 | 7722 4160 | /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits |
**** FOUND 10:54:58.33 -24:19:10.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 3.675 3536858843308390272 163.74238755299 -24.32035655833 14.2549 13.6973 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.675#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71322_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048
The candidate 71322_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
| Discovery image 2 | 2026 02 27.21439 | 2461098.71439 | 13.39 | 10:02:51.88 -29:42:51.5 | 0733 0753 | /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits |
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 71366_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048
The candidate 71366_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
| Discovery image 2 | 2026 02 27.21439 | 2461098.71439 | 14.23 | 10:48:48.37 -28:03:22.1 | 6820 1920 | /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits |
**** FOUND 10:48:48.37 -28:03:23.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.08, MAG_FAINT_SEARCH_LIMIT=15.06)GAIADR2_OUTPUT=# 0.520 5457282035820081664 162.20142886031 -28.05649353831 14.1716 13.6559 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.520#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71432_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048
The candidate 71432_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
| Discovery image 2 | 2026 02 27.21439 | 2461098.71439 | 13.97 | 10:48:45.63 -28:14:27.0 | 6812 1808 | /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits |
**** FOUND 10:48:45.76 -28:14:26.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 0.993 5456521792248174720 162.19088303790 -28.24097712585 14.1931 13.6983 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.993#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71458_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048
The candidate 71458_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
| Discovery image 2 | 2026 02 27.21439 | 2461098.71439 | 14.07 | 10:56:19.60 -26:08:15.5 | 7871 3053 | /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits |
**** FOUND 10:56:19.56 -26:08:15.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.06, MAG_FAINT_SEARCH_LIMIT=15.04)GAIADR2_OUTPUT=# 1.454 5457980603660553984 164.08194915915 -26.13753323036 14.3311 13.8069 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.454#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71551_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048
The candidate 71551_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
| Discovery image 2 | 2026 02 27.21439 | 2461098.71439 | 14.25 | 11:06:09.26 -20:45:17.9 | 9409 6284 | /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits |
**** FOUND 11:06:09.28 -20:45:18.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)GAIADR2_OUTPUT=# 1.152 3551311648777482624 166.53832507760 -20.75503790309 13.3959 12.8362 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.152#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 35199_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048
The candidate 35199_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
| Discovery image 3 | 2026 02 27.21439 | 2461098.71439 | 12.58 | 10:03:08.66 -24:41:30.9 | 0569 3813 | /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits |
Rejecting candidate due to large distance (34.2") between the two second-epoch detections
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Considering the candidate 42352_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048
The candidate 42352_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
| Discovery image 3 | 2026 02 27.21439 | 2461098.71439 | 12.28 | 11:00:37.57 -21:55:33.7 | 8576 5593 | /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits |
Rejecting candidate due to large distance (33.0") between the two second-epoch detections
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Considering the candidate 30470_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048
Preparing report for the candidate 30470_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048
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Considering the candidate 32555_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048
The candidate 32555_Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048 did not pass the final checks
| Discovery image 3 | 2026 02 27.21439 | 2461098.71439 | 12.33 | 10:25:56.13 -25:25:25.8 | 3732 3506 | /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Hya-10-Q2b1x1_235145_TTUQ2b1x1_5387_BdNUSRc6/Hya-10-Q2b1x1_2026-02-26_23-08-33_20.00sec_-14.90C_LIGHT_0048.fits |
Rejecting candidate due to large distance (33.5") between the two second-epoch detections
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 7s
Prepared the HTML report for the field Hya-10-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
10:39:33.16 -25:50:36.5
########### Completed Hya-10-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
10:39:33.16 -25:50:36.5
###################################################################################
10:39:33.16 -25:50:36.5 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
10:39:33.16 -25:50:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
10:39:33.16 -25:50:36.5 -- a known variable star
Found 0 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
1 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
Adding identified Gaia sources from exclusion_list_gaiadr2.txt
exclusion_list_apass.txt NOT FOUND
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
10:39:33.16 -25:50:36.5
10:36:24.71 -24:34:44.1
10:11:16.53 -27:14:12.6
09:58:17.86 -30:16:47.2
10:42:49.73 -25:23:44.2
11:01:42.11 -24:49:04.6
10:02:22.94 -30:04:50.4
11:06:13.89 -23:38:37.0
11:05:09.59 -22:03:18.7
11:07:47.39 -30:34:34.1
10:07:05.40 -27:50:40.0
10:12:37.20 -30:46:08.9
10:49:09.67 -22:11:14.3
10:43:34.38 -29:59:57.7
11:01:25.47 -28:10:11.8
11:00:38.04 -27:29:06.1
10:49:45.36 -28:55:08.0
10:53:19.02 -30:05:56.6
10:58:17.58 -25:00:39.9
11:01:24.11 -29:36:01.2
10:54:58.33 -24:19:10.3
10:48:48.37 -28:03:23.0
10:48:45.76 -28:14:26.8
10:56:19.56 -26:08:15.2
11:06:09.28 -20:45:18.2
####################################################
The observatory MPC code is 500
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461098.71384287 -observatory 500
23:26:22.83 -00:23:11.4 Mercury (1.2mag)
23:27:42.68 -04:59:21.9 Venus (-3.9mag)
21:58:15.96 -13:32:56.2 Mars (1.1mag)
07:05:04.81 +22:56:17.1 Jupiter (-2.5mag)
00:07:35.60 -01:30:05.7 Saturn (1.0mag)
03:40:21.89 +19:23:03.6 Uranus (5.7mag)
00:04:19.71 -00:57:21.0 Neptune (7.8mag)
20:29:43.54 -22:58:11.2 Pluto (14.5mag)
07:01:42.79 +27:01:34.1 Moon (-11.3mag)
-rw-r--r-- 1 apache apache 362 Feb 27 03:37 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461098.71384287:
07:05:01.24 +22:56:26.4 Io (5.4mag)
07:04:56.78 +22:56:29.0 Europa (5.6mag)
07:04:45.21 +22:56:48.3 Ganymede (5.0mag)
07:05:31.81 +22:55:18.0 Callisto (6.2mag)
07:08:33.39 +23:10:12.4 Himalia (15.1mag)
07:05:01.66 +22:56:19.9 Thebe (15.9mag)
07:07:55.82 +23:21:42.8 Elara (17.0mag)
07:00:54.23 +24:01:35.0 Pasiphae (17.1mag)
07:14:04.50 +22:45:43.9 Carme (18.1mag)
00:07:35.31 -01:29:45.9 Titan (8.8mag)
00:07:41.06 -01:30:01.2 Rhea (10.1mag)
00:07:43.39 -01:30:52.4 Iapetus (11.5mag)
00:07:50.36 -01:30:12.6 Hyperion (14.8mag)
00:09:38.59 -01:17:21.2 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Feb 27 03:38 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461098.71384287:
09:28:00.40 +24:03:18.7 JWST
21:07:03.51 -22:30:45.9 Chandra
07:54:25.76 -27:56:54.8 XMM-Newton
-rw-r--r-- 1 apache apache 96 Feb 27 03:37 spacecraft.txt
############################################################
Positions of bright comets (listed at http://astro.vanbuitenen.nl/comets and http://aerith.net/comet/weekly/current.html ) from JPL HORIZONS for JD(UT)2461098.71384287 at 500
17:09:29.93 -11:06:32.2 17.4mag 10P/Tempel 2
03:42:28.36 +29:15:54.9 18.0mag 123P/West-Hartley
08:16:40.36 +59:04:23.5 18.3mag 124P/Mrkos
21:36:40.03 -06:10:43.7 22.0mag 141P/Machholz
01:32:27.27 +13:19:40.4 17.7mag 145P/Shoemaker-Levy 5
10:58:08.19 +31:05:29.6 18.0mag 164P/Christensen
09:30:23.32 -33:36:03.9 18.0mag 195P/Hill
15:50:57.63 -06:05:17.8 19.5mag 210P/Christensen
18:40:06.95 -21:04:56.2 17.2mag 218P/LINEAR
16:29:54.70 -18:01:41.9 15.2mag 235P/LINEAR
04:03:52.95 +28:38:43.5 17.9mag 240P/NEAT
15:22:48.32 +06:17:20.5 14.9mag 24P/Schaumasse
11:21:25.38 -03:14:46.7 17.3mag 29P/Schwassmann-Wachmann 1
07:03:35.62 +27:25:31.3 19.5mag 407P/PanSTARRS-Fuls
17:15:16.28 -11:15:42.4 17.6mag 40P/Vaisala 1
10:58:51.79 -08:32:35.0 16.6mag 43P/Wolf-Harrington
13:25:16.39 -06:03:12.7 20.2mag 489P/Denning
04:38:24.84 +48:10:19.6 17.8mag 493P/2024 Q2 (LONEOS)
06:06:55.46 +46:34:34.5 17.6mag 63P/Wild 1
23:24:43.66 -01:11:09.1 16.2mag 78P/Gehrels 2
20:20:22.57 -21:30:08.6 14.9mag 88P/Howell
20:47:42.75 -28:44:50.9 0.0mag P/2010 H3 (SOHO)
15:30:10.63 -29:24:04.0 18.6mag P/2023 S1 (PanSTARRS)
04:44:08.10 -72:18:18.1 16.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:29:11.80 +31:13:44.2 18.2mag C/2017 K2 (PanSTARRS)
20:09:20.70 -65:21:55.1 18.1mag C/2020 V2 (ZTF)
17:23:41.61 +04:53:45.6 16.3mag C/2021 G2 (ATLAS)
03:39:51.80 +24:43:12.4 15.8mag C/2022 N2 (PanSTARRS)
09:06:33.13 +30:13:00.7 15.3mag C/2022 QE78 (ATLAS)
08:34:13.21 -05:56:03.0 16.7mag C/2022 R6 (PanSTARRS)
23:59:25.50 +48:40:11.8 18.0mag C/2023 C2 (ATLAS)
09:45:37.20 -20:00:16.0 17.5mag C/2023 F3 (ATLAS)
20:44:38.27 +61:15:43.4 17.3mag C/2023 H5 (Lemmon)
19:34:57.70 -03:26:26.3 16.0mag C/2023 R1 (PANSTARRS)
02:50:43.92 +35:38:44.6 18.5mag C/2023 RS61 (PanSTARRS)
21:09:35.09 +81:28:27.9 18.0mag C/2023 X2 (Lemmon)
06:32:20.45 +63:54:12.1 17.4mag C/2024 A1 (ATLAS)
02:30:44.08 -17:42:18.3 11.5mag C/2024 E1 (Wierzchos)
11:40:54.64 -01:36:32.9 18.1mag C/2024 G2 (ATLAS)
19:33:05.85 +00:49:58.1 18.9mag C/2024 G4 (PanSTARRS)
16:36:54.36 -01:02:27.7 17.7mag C/2024 G6 (ATLAS)
19:56:53.19 +04:11:57.7 15.5mag C/2024 J3 (ATLAS)
02:50:03.22 -30:37:17.5 15.4mag C/2024 T5 (ATLAS)
16:09:32.62 -60:08:37.8 15.7mag C/2025 A6 (Lemmon)
04:50:04.72 +60:16:17.2 16.7mag C/2025 J1 (Borisov)
15:52:30.45 -08:32:02.1 14.7mag C/2025 L1 (ATLAS)
02:24:44.88 -19:47:28.9 16.8mag C/2025 Q3 (ATLAS)
02:16:00.42 +17:45:19.3 21.3mag C/2025 R2 (SWAN)
22:22:38.53 +17:48:20.4 16.1mag C/2025 R3 (PANSTARRS)
21:51:18.28 -17:54:19.3 22.1mag C/2025 T1 (ATLAS)
02:55:08.65 -18:04:48.2 18.1mag C/2026 A1 (MAPS)
21:21:50.36 +23:08:38.3 17.0mag C/2026 B2 (Sun-Gao)
-rw-r--r-- 1 apache apache 2.6K Feb 27 03:38 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
18:03:39.37 +19:58:46.70 ASASSN-26be 2026-02-25.58 14.8
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.49 -48:05:16.60 SN2026dez 2026-02-19.31 15.91
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.08 -11:25:16.30 AT2026bzh 2026-02-12.45 17.3
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
06:26:33.34 -54:06:39.90 AT2026cih 2026-02-8.06 17.26
23:08:59.40 -88:59:11.60 SN 2026bsu 2026-02-8.03 16.02
01:04:14.94 -62:31:02.30 SN 2026azk 2026-02-8.04 16.41
08:44:55.41 +64:55:09.90 SN 2026anq 2026-02-7.16 17.62
12:37:42.99 +33:26:05.40 SN 2026bnm 2026-02-7.29 16.74
00:12:55.45 +33:21:25.90 SN2026cbh 2026-02-7.09 16.33
08:02:12.64 -04:14:20.90 SN 2026auh 2026-02-7.11 16.64
18:03:52.67 -31:27:26.00 TCP J18035290-3127298 2026-02-7.37 15.76
12:18:03.59 +50:27:10.20 SN 2026bjz 2026-02-7.25 16.48
07:51:51.12 +55:05:27.60 SN 2026ail 2026-02-6.21 16.85
08:10:56.38 +36:49:42.80 AT2026bsa 2026-02-6.29 17.47
04:43:45.47 -15:49:01.00 SN2026azr 2026-02-5.24 16.96
06:14:48.48 -34:20:08.90 ASASSN-26ap 2026-02-5.2 13.77
02:42:33.90 -27:21:02.60 SN 2026aip 2026-02-4.09 15.85
00:43:12.26 +38:35:47.90 AT2026brt 2026-02-3.12 14.92
14:34:27.21 +21:56:59.90 SN2026atb 2026-01-29.32 15.59
13:12:04.11 -60:56:12.40 ASASSN-26ao 2026-01-28.35 15.61
13:00:36.49 -06:28:26.00 SN2026azd 2026-01-28.23 15.69
10:33:50.27 -31:00:53.40 SN 2026ayz 2026-01-25.11 15.3
05:14:22.36 -60:47:20.70 SN 2026apb 2026-01-24.08 17.35
06:39:26.57 -21:49:19.60 AT2026afe 2026-01-23.11 16.17
09:27:23.49 -32:00:30.90 SN 2023kuy 2026-01-21.16 15.43
09:38:44.42 -20:00:54.30 SN2026afi 2026-01-20.24 17.43
06:30:51.41 -74:35:46.80 AT2026ahr 2026-01-20.09 16.98
13:33:03.15 -16:14:28.70 SN2026amc 2026-01-20.29 16.9
06:57:11.13 -17:24:42.80 ASASSN-26an 2026-01-19.31 13.99
17:41:29.59 +68:57:34.90 2026abj 2026-01-18.64 17.02
10:22:24.99 +04:00:02.20 SN 2026kc 2026-01-18.61 16.1
12:42:03.30 +00:41:41.80 SN 2026pg 2026-01-18.5 17.44
03:36:21.80 -31:44:39.30 AT2025aibn 2026-01-17.04 16.7
13:45:00.71 -32:34:53.00 AT2026yi 2026-01-17.26 16.22
09:27:07.17 +62:45:24.20 AT2026nu 2026-01-17.29 17.09
12:38:41.73 +07:36:37.40 SN 2025afcr 2026-01-17.49 17.11
12:12:12.65 +13:13:18.50 SN 2026acd 2026-01-17.3 16.15
16:21:54.73 -63:36:53.10 ASASSN-26al 2026-01-17.36 15.34
15:33:45.22 -22:11:07.90 ASASSN-26aj 2026-01-16.51 14
12:27:08.33 -58:19:36.10 ASASSN-26ak 2026-01-16.2 13.94
17:21:53.10 +04:39:07.10 ASASSN-26ai 2026-01-16.67 14.83
14:46:54.08 -64:04:30.10 ASASSN-26ah 2026-01-15.07 16.84
23:02:43.24 +20:04:53.00 SN2025ajvh 2026-01-15.07 16.03
14:12:27.38 -30:12:29.10 ASASSN-26ag 2026-01-14.27 15.35
14:33:53.58 +05:27:35.40 SN 2025ajnc 2026-01-14.32 15.79
01:43:00.31 -34:11:40.60 AT2025afcm 2026-01-13.08 0.45
00:26:17.71 -52:11:38.60 AT2025ahal 2026-01-11.06 17.57
00:51:36.17 +29:42:40.10 SN2025ahxd 2026-01-11.21 15
10:19:19.14 -37:54:58.30 AT2025ahrt 2026-01-10.26 -0.54
14:37:48.78 +15:51:04.20 SN2025ajng 2026-01-9.42 16.35
05:01:03.70 -08:34:13.20 SN2026A 2026-01-9.28 16.83
00:02:52.11 +13:05:42.90 SN2025ajvg 2026-01-9.13 15.89
08:37:09.62 -02:18:08.80 SN2025aigm 2026-01-9.55 17.66
09:52:50.71 +39:36:55.70 SN2025ahyt 2026-01-9.37 16.97
11:22:19.08 -27:21:40.90 AT2026ta 2026-01-9.32 15.88
14:35:00.21 +00:59:11.40 SN 2025ahsa 2026-01-8.35 -2
09:25:42.42 +22:20:06.10 SN2025ahkt 2026-01-8.03 15.88
22:39:53.44 +34:53:50.00 SN 2025aikz 2026-01-7.09 16.3
08:21:20.95 +20:52:01.60 SN 2025aiks 2026-01-7.13 15.82
07:35:31.38 +09:10:32.40 AT2025ajvk 2026-01-7.12 -1.82
02:50:07.71 -16:37:02.30 AT2026nl 2026-01-7.16 14.19
14:05:12.75 -33:46:00.80 SN 2025ajmj 2026-01-7.31 14.93
12:35:08.33 +28:03:22.70 SN 2025aiaj 2026-01-5.44 15.76
05:30:00.47 -66:43:29.40 ASASSN-26af 2026-01-5.12 14.38
14:05:05.13 -44:14:24.00 ASASSN-26ac 2026-01-5.3 16.01
11:29:16.57 +20:35:09.00 AT2025alco 2026-01-4.39 15.93
16:42:59.28 +26:21:02.80 ASASSN-26ae 2026-01-4.52 14.31
04:13:46.60 -05:02:16.60 ASASSN-26ad 2026-01-4.32 14.58
05:00:01.32 -57:14:29.70 ASASSN-25fj/ASASSN-26ab 2026-01-1.19 13.38
13:53:51.35 -17:55:38.10 ASASSN-25fg 2025-12-23.33 16.66
06:18:15.27 +15:47:38.10 AT2025ahtd 2025-12-23.31 16.96
-rw-r--r-- 1 apache apache 5.7K Feb 27 03:37 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:41:01.11 +41:59:28.2 PNV J00410111+4159282 2026-01-06.1994 18.7mag
00:42:52.01 +41:14:29.2 PNV J00425201+4114292 2026-01-08.7863 18.37Cmag
02:50:07.72 -16:37:02.3 TCP J02500772-1637023 2026-01-06.6352 14.53Cmag
00:42:58.52 +41:14:44.2 PNV J00425852+4114442 2026-01-13.4991 16.89Cmag
14:47:33.95 -10:02:56.8 TCP J14473395-1002568 2026-01-13.8185 14.0mag
15:33:45.28 -22:11:07.3 TCP J15334528-2211073 2026-01-16.8451 14.9mag
22:34:01.26 +39:53:32.8 TCP J22340126+3953328 2026-01-17.5738 16.79Cmag
00:42:52.36 +41:16:13.3 PNV J00425236+4116133 2026-01-18.5502 17.41Cmag
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
-rw-r--r-- 1 apache apache 187K Feb 27 03:37 tocp_transients_list.txt