This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 03 19.3234 2461118.8234 13.42 08:57:51.45 +01:42:27.8
226.93697 28.67153 galactic Hya Second-epoch detections are separated by 2.7" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:57:51.45 +01:42:27.8 (user input) | T | P | (position from user input) SpType: G7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8234,13.42,0.05,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
target 20260319.3234 13.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:57:51.45 +01:42:27.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20_00sec_-15_00C_LIGHT_0045_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20_00sec_-15_00C_LIGHT_0044_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20_00sec_-15_00C_LIGHT_0044_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 577838719546689664,2461118.8234,12.75,0.05,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
Gaia DR3 577838719546689664 20260319.3234 12.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:56:34.11 +02:31:40.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20_00sec_-15_00C_LIGHT_0045_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20_00sec_-15_00C_LIGHT_0044_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20_00sec_-15_00C_LIGHT_0045_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20_00sec_-14_90C_LIGHT_0506_fits__*pix.png resample_wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20_00sec_-15_00C_LIGHT_0044_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.90316561 23.12.2025 09:40:23.509 /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
First image: 2461032.90316561 23.12.2025 09:40:23.509 /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
Last image: 2461118.82364564 19.03.2026 07:45:52.983 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.65
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 10374
Objects passed selection criteria: 10370
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 9738.25
Average stars matched: 9525 (97.8102 %)
Memory usage VmPeak: 115784 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Mar 11 15:05:24 CDT 2026
VaST build number 1.0rc88-349-g45f03b26
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 19 03:02:00 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.90316561 23.12.2025 09:40:23.509 /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
First image: 2461032.90316561 23.12.2025 09:40:23.509 /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
Last image: 2461118.82364564 19.03.2026 07:45:52.983 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 117
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.39
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 17 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 61624
Objects passed selection criteria: 61500
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 56688.8
Average stars matched: 54993.2 (97.0091 %)
Memory usage VmPeak: 160556 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Mar 11 15:05:24 CDT 2026
VaST build number 1.0rc88-349-g45f03b26
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 19 03:02:51 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits
SExtractor catalog cache: saved Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat to cache
SExtractor catalog cache: saved Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.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-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.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: 2461118.82310315
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-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits exists and is non-empty
Saving wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits to local_wcs_cache/
'wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits' -> 'local_wcs_cache/wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits'
wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits exists and is non-empty
Saving wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits to local_wcs_cache/
'wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits' -> 'local_wcs_cache/wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits'
wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits exists and is non-empty
Saving wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits to local_wcs_cache/
'wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits' -> 'local_wcs_cache/wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits'
wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits exists and is non-empty
Saving wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits to local_wcs_cache/
'wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits' -> 'local_wcs_cache/wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.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 09:25:43.993 -02:00:09.35
Second-epoch image center 09:25:50.941 -02:01:32.31
Angular distance between the image centers 0.04 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 09:25:43.993 -02:00:09.35
Second-epoch image center 09:25:49.570 -02:01:45.45
Angular distance between the image centers 0.04 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 09:25:50.941 -02:01:32.31
Second-epoch second image center 09:25:49.570 -02:01:45.45
Angular distance between the image centers 0.00678 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-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits &> /tmp/tmp.BYrcfk4cnO
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits &> /tmp/tmp.TVvCMl2E4r
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits &> /tmp/tmp.GJk1q9dS7Y
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits &> /tmp/tmp.29ULuqRIF7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.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-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits and wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.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-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits and wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat
Found non-empty wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits and wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat
The reference image (wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits) and catalog (wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat) found
'wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.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 5565 out of 10420 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.932573
a=0.000000 b=1.000000 c=22.932573
From vast_summary.log: estimated ref. image limiting mag.: -7.65
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.28
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.28
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
2.0 pix Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
2.4 pix fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits
2.4 pix fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits
Limiting magnitude estimates:
15.3 mag. Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
15.3 mag. Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
15.0 mag. fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits
15.0 mag. fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 12.1 (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.BYrcfk4cnO (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-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.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-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.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-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits' -> 'wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
WCS_IMAGE_NAME=wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
WCS-calibrated image found: wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
Checking if the catalog wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat corresponding to the image wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits alredy exist and is non-empty...
Catalog wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat corresponding to the image wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
WCS catalog name: wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=740, passed=10420
Got 10420 stars (including 9668 good ones) from the SExtractor catalog wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat
util/solve_plate_with_UCAC5 got 10420 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 938 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: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.27"
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 937 stars left (next iteration limit 1030)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits -region wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.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.TVvCMl2E4r (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-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.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-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.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-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits' -> 'wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
WCS_IMAGE_NAME=wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
WCS-calibrated image found: wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
Checking if the catalog wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits.cat corresponding to the image wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits alredy exist and is non-empty...
Catalog wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits.cat corresponding to the image wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
WCS catalog name: wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=743, passed=10444
Got 10444 stars (including 9684 good ones) from the SExtractor catalog wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits.cat
util/solve_plate_with_UCAC5 got 10444 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 937 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: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.27"
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 936 stars left (next iteration limit 1029)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits -region wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.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.GJk1q9dS7Y (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits
WCS_IMAGE_NAME=wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits
WCS-calibrated image found: wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits
Checking if the catalog wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits.cat corresponding to the image wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits.cat corresponding to the image wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits
WCS catalog name: wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=517, passed=9189
Got 9189 stars (including 8660 good ones) from the SExtractor catalog wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits.cat
util/solve_plate_with_UCAC5 got 9189 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 927 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: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.50"
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 927 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.50"
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 927 stars left (next iteration limit 1019)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits -region wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.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.29ULuqRIF7 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits
WCS_IMAGE_NAME=wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits
WCS-calibrated image found: wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits
Checking if the catalog wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits.cat corresponding to the image wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits.cat corresponding to the image wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits
WCS catalog name: wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=508, passed=9157
Got 9157 stars (including 8641 good ones) from the SExtractor catalog wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits.cat
util/solve_plate_with_UCAC5 got 9157 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 929 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: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
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 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.49"
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 929 stars left (next iteration limit 1021)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits -region wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits'
Saving fully-calibrated image wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits'
Saving fully-calibrated image wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits'
Saving fully-calibrated image wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits'
Preparing the HTML report for the field Hya-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20650.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 20553_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 20553_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 09:24:50.34 -06:47:31.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20650_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 20650_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 09:03:53.66 -03:37:50.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 0.377 5762551543665508736 135.97362867461 -03.63087211275 12.2249 11.7891 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.377#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06636_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 06636_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 08:58:16.68 -00:49:53.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04227_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 04227_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 08:57:46.77 -03:16:53.7 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Hya-04-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 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits
SExtractor catalog cache: saved Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat to cache
SExtractor catalog cache: saved Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.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-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
Creating symlink local_wcs_cache/wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.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-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits exists and is non-empty
wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits exists and is non-empty
wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits exists and is non-empty
wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.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 09:25:43.993 -02:00:09.35
Second-epoch image center 09:25:50.941 -02:01:32.31
Angular distance between the image centers 0.04 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 09:25:43.993 -02:00:09.35
Second-epoch image center 09:25:49.570 -02:01:45.45
Angular distance between the image centers 0.04 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 09:25:50.941 -02:01:32.31
Second-epoch second image center 09:25:49.570 -02:01:45.45
Angular distance between the image centers 0.00678 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-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits &> /tmp/tmp.DlnVi1HheF
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits &> /tmp/tmp.ZUsh6uFNZ0
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits &> /tmp/tmp.c0Qpp7GRgl
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits &> /tmp/tmp.KptDiDjJTN
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.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-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits and wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.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-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits and wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat
Found non-empty wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits and wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat
The reference image (wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits) and catalog (wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat) found
'wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat' -> 'wcsmag.cat'
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 5627 out of 64348 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.821408
a=0.000000 b=1.000000 c=22.821408
From vast_summary.log: estimated ref. image limiting mag.: -7.39
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.43
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.43
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 51 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
1.9 pix Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
2.3 pix fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits
2.3 pix fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits
Limiting magnitude estimates:
15.4 mag. Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
15.4 mag. Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
15.1 mag. fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits
15.1 mag. fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 14.4 (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.DlnVi1HheF (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-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.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-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.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-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits' -> 'wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
WCS_IMAGE_NAME=wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
WCS-calibrated image found: wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
Checking if the catalog wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat corresponding to the image wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits alredy exist and is non-empty...
Catalog wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat corresponding to the image wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
WCS catalog name: wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=3271, passed=64335
Got 64335 stars (including 60948 good ones) from the SExtractor catalog wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat
util/solve_plate_with_UCAC5 got 64335 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 942 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 942 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 - 942 stars left (next iteration limit 1036)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits -region wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.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.ZUsh6uFNZ0 (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-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.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-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.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-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits' -> 'wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
WCS_IMAGE_NAME=wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
WCS-calibrated image found: wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
Checking if the catalog wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits.cat corresponding to the image wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits alredy exist and is non-empty...
Catalog wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits.cat corresponding to the image wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
WCS catalog name: wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=3228, passed=64125
Got 64125 stars (including 60786 good ones) from the SExtractor catalog wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits.cat
util/solve_plate_with_UCAC5 got 64125 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 943 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: 0.30"
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 943 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: 0.29"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits -region wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.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.c0Qpp7GRgl (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits
WCS_IMAGE_NAME=wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits
WCS-calibrated image found: wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits
Checking if the catalog wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits.cat corresponding to the image wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits.cat corresponding to the image wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits
WCS catalog name: wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=2577, passed=50059
Got 50059 stars (including 47426 good ones) from the SExtractor catalog wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits.cat
util/solve_plate_with_UCAC5 got 50059 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 926 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
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 926 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.49"
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 926 stars left (next iteration limit 1018)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits -region wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.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.KptDiDjJTN (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits
WCS_IMAGE_NAME=wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits
WCS-calibrated image found: wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits
Checking if the catalog wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits.cat corresponding to the image wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits.cat corresponding to the image wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits
WCS catalog name: wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=28, blended=2469, passed=49816
Got 49816 stars (including 47277 good ones) from the SExtractor catalog wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits.cat
util/solve_plate_with_UCAC5 got 49816 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
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 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.48"
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 929 stars left (next iteration limit 1021)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits -region wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/wcs_Hya-04-Q2b1x1_2025-12-23_03-40-23_20.00sec_-14.90C_LIGHT_0506.fits
Saving fully-calibrated image wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/wcs_Hya-04-Q2b1x1_2025-12-23_03-41-00_20.00sec_-15.00C_LIGHT_0507.fits
Saving fully-calibrated image wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-06_20.00sec_-15.00C_LIGHT_0044.fits
Saving fully-calibrated image wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-04-Q2b1x1_025945_TTUQ2b1x1_9976_mvehbqzi/wcs_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045.fits
Preparing the HTML report for the field Hya-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out78817.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78830.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78834.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78839.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78840.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78842.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78846.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78847.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78849.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78850.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78857.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78858.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78862.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78864.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78870.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78872.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78883.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78887.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78888.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78915.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78935.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78942.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79268.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79310.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79336.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79440.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79491.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79542.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79552.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79555.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79747.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out79314.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out78918.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78936.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 16s
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 78817_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 78817_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 09:54:25.97 -02:54:07.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.48, MAG_FAINT_SEARCH_LIMIT=15.46)GAIADR2_OUTPUT=# 0.527 3823510698718691328 148.60833893112 -02.90203868856 14.5396 13.9188 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.527#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78825_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 78825_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 09:45:12.07 -04:29:14.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78830_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 78830_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 09:49:38.47 -03:24:56.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.36, MAG_FAINT_SEARCH_LIMIT=15.34)GAIADR2_OUTPUT=# 3.566 3826014080536760832 147.41088558098 -03.41648806920 14.4319 13.7834 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.566#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78834_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 78834_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 09:44:11.49 -00:21:21.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 1.935 3828043641562579200 146.04807004212 -00.35547124352 14.5748 14.0792 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.935#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78839_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 78839_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 09:24:33.99 -03:28:23.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 0.369 3837295344715768960 141.14163308613 -03.47326872777 14.2738 13.7680 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.369#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78840_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 78840_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 09:45:22.25 -02:30:01.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.36, MAG_FAINT_SEARCH_LIMIT=15.34)GAIADR2_OUTPUT=# 1.801 3826366096056260992 146.34227344785 -02.50077599481 14.0750 13.3332 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.801#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78842_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 78842_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 09:53:37.78 +01:03:30.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 0.883 3834563711155611264 148.40718284074 +01.05840765819 14.0660 13.5630 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.883#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78846_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 78846_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 08:56:18.07 +00:01:18.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 1.069 3074495065453383296 134.07558248653 +00.02175419962 13.4734 13.0296 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.069#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78847_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 78847_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 09:45:55.17 +02:38:55.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)
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Considering the candidate 78849_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 78849_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 08:59:03.48 +01:36:07.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.09, MAG_FAINT_SEARCH_LIMIT=15.07)GAIADR2_OUTPUT=# 2.333 576955704334806656 134.76394799081 +01.60250645366 13.5778 13.0945 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.333#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78850_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 78850_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 08:56:28.14 +02:46:57.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)GAIADR2_OUTPUT=# 5.662 577858850057619840 134.11871563163 +02.78192506771 13.5184 13.1021 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.662#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78857_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 78857_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 08:56:04.49 +02:01:08.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)GAIADR2_OUTPUT=# 2.734 577655547781467648 134.01927146266 +02.01854559183 13.3541 12.7747 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.734#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78858_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 78858_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 09:26:08.84 +01:38:38.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)GAIADR2_OUTPUT=# 1.276 3844461411749646848 141.53649613376 +01.64383461855 14.2283 13.7223 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.276#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78862_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 78862_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 08:56:48.17 +01:50:29.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 3.819 577634966298181120 134.20166184366 +01.84106197754 13.3554 12.7631 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.819#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78864_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 78864_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 09:01:41.44 +01:19:04.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 1.388 576700828091079808 135.42272848996 +01.31756397831 13.7038 13.2916 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.388#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78870_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 78870_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 09:33:08.89 -01:11:35.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 0.493 3839647745549127808 143.28699892259 -01.19321351693 13.8925 13.2149 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.493#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78872_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 78872_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 08:57:04.12 +01:07:49.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)
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Considering the candidate 78883_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 78883_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 08:56:28.00 +03:04:25.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 0.603 578061091478367232 134.11675212991 +03.07360578965 13.0549 12.4358 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.603#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78884_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 78884_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 09:48:22.60 -00:05:42.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78887_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 78887_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 09:00:05.08 +02:50:02.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 3.183 578179563855879936 135.02205196909 +02.83414936333 13.1020 12.4292 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.183#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78888_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 78888_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 08:54:41.86 -05:35:52.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 2.694 5760695464958841728 133.67516336066 -05.59777422151 13.3406 12.7222 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.694#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78915_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 78915_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 09:25:31.63 -01:28:44.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 1.062 3838911214491679104 141.38170967323 -01.47922778435 13.2758 12.8288 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.062#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78918_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
Preparing report for the candidate 78918_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
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Considering the candidate 78935_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 78935_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 08:56:16.27 +03:08:03.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 4.665 578073499638890880 134.06649817761 +03.13427227311 12.0041 11.3046 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.665#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78936_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
Preparing report for the candidate 78936_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
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Considering the candidate 78940_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 78940_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 09:44:13.35 +01:49:25.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78942_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 78942_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 08:57:25.52 +02:22:07.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 5.850 577785702470484480 134.35470749424 +02.36878751776 11.6050 10.9769 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.850#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78943_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 78943_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 09:55:36.25 +00:10:10.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79089_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 79089_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 09:51:09.19 -00:50:57.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79106_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 79106_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 09:52:17.12 +00:05:39.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 79129_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 79129_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 09:26:14.96 -01:28:51.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 79202_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 79202_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 09:55:15.90 -03:56:37.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79268_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 79268_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 09:16:46.47 -04:35:41.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 0.884 5758844230974725760 139.19360404991 -04.59505028515 13.5473 12.8887 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.884#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79310_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 79310_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 08:59:45.07 -04:47:03.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 5.302 5760854619266109184 134.93657609169 -04.78511555741 13.3937 12.4453 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.302#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79314_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 79314_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 09:45:53.40 -00:16:06.8 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)
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Considering the candidate 79336_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 79336_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 09:17:30.73 +00:31:52.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 1.904 3842609765449299712 139.37780884845 +00.53069164338 13.7668 13.2339 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.904#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79347_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 79347_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 09:48:20.62 -06:15:21.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79354_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 79354_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 09:44:50.57 -00:37:42.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79403_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 79403_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 09:32:45.23 +01:52:59.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 79436_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 79436_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 09:34:17.30 -07:03:44.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79440_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 79440_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 09:28:15.09 -03:33:52.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 0.725 3825620352295019648 142.06276694196 -03.56486465284 14.2528 13.7470 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.725#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79491_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 79491_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 09:10:05.23 -04:10:08.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.19, MAG_FAINT_SEARCH_LIMIT=15.17)GAIADR2_OUTPUT=# 2.439 5759625880662860160 137.52116713057 -04.16887231218 14.2957 13.6603 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.439#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79542_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 79542_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 09:22:15.69 +02:37:23.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.32, MAG_FAINT_SEARCH_LIMIT=15.30)GAIADR2_OUTPUT=# 2.927 3845519210654996992 140.56462766551 +02.62295594575 14.5277 14.0520 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.927#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79552_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 79552_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 09:05:22.56 -02:37:27.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)GAIADR2_OUTPUT=# 2.974 5763051993254615424 136.34329334696 -02.62476248218 14.1023 13.6012 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.974#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79555_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 79555_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 09:12:11.63 -01:17:24.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 2.069 3841799768976969600 138.04832171634 -01.28946959616 14.3233 13.8428 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.069#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79747_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 79747_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 09:54:13.34 -06:11:36.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.49, MAG_FAINT_SEARCH_LIMIT=15.47)GAIADR2_OUTPUT=# 0.749 3821602083971927552 148.55543189764 -06.19364365947 14.5988 14.0616 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.749#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79796_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 79796_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
Rejecting candidate due to large distance (23.2") between the two second-epoch detections
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Considering the candidate 25919_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 25919_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 08:57:46.77 -03:16:53.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75354_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 75354_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
Rejecting candidate due to large distance (24.5") between the two second-epoch detections
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Considering the candidate 52576_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 52576_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks
**** FOUND 08:58:16.69 -00:49:53.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 03064_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045
The candidate 03064_fd_Hya-04-Q2b1x1_2026-03-19_02-45-52_20.00sec_-15.00C_LIGHT_0045 did not pass the final checks