This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG
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 20.1694 2461119.6694 13.21 11:09:45.75 -23:01:01.2
274.41317 34.16281 galactic Crt Second-epoch detections are separated by 8.8" and 3.4 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 | Gaia DR3 3538717052320011392 | 11:09:45.28 -23:01:00.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
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
Gaia DR3 3538717052320011392,2461119.6694,13.21,0.05,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 3538717052320011392 20260320.1694 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 11:09:45.75 -23:01:01.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20_00sec_-14_90C_LIGHT_0133_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20_00sec_-15_00C_LIGHT_0132_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20_00sec_-15_00C_LIGHT_0132_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
target,2461119.6694,14.18,0.05,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 20260320.1694 14.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:43:53.95 -13:53:24.8 ;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-09-Q2b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20_00sec_-14_90C_LIGHT_0133_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20_00sec_-15_00C_LIGHT_0132_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20_00sec_-14_90C_LIGHT_0530_fits__*pix.png resample_wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20_00sec_-15_00C_LIGHT_0132_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.91964973 23.12.2025 10:04:07.737 /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
First image: 2461032.91964973 23.12.2025 10:04:07.737 /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
Last image: 2461119.66962898 20.03.2026 04:04:05.944 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.97
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 2 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): 7456
Objects passed selection criteria: 7451
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: 7130.5
Average stars matched: 7016.75 (98.4047 %)
Memory usage VmPeak: 113500 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 23:38:11 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: 2461032.91964973 23.12.2025 10:04:07.737 /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
First image: 2461032.91964973 23.12.2025 10:04:07.737 /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
Last image: 2461119.66962898 20.03.2026 04:04:05.944 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 65
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.73
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 12 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): 44962
Objects passed selection criteria: 44890
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: 42948.8
Average stars matched: 41433.8 (96.4725 %)
Memory usage VmPeak: 145324 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 23:38:57 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-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits
SExtractor catalog cache: saved Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat to cache
SExtractor catalog cache: saved Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.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: 2461119.66909497
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits exists and is non-empty
Saving wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits to local_wcs_cache/
'wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits' -> 'local_wcs_cache/wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits'
wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits exists and is non-empty
Saving wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits to local_wcs_cache/
'wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits' -> 'local_wcs_cache/wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits'
wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits exists and is non-empty
Saving wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits to local_wcs_cache/
'wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits' -> 'local_wcs_cache/wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits'
wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits exists and is non-empty
Saving wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits to local_wcs_cache/
'wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits' -> 'local_wcs_cache/wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 10:39:59.375 -17:59:54.09
Second-epoch image center 10:39:47.908 -17:59:20.14
Angular distance between the image centers 0.05 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 10:39:59.375 -17:59:54.09
Second-epoch image center 10:39:45.894 -17:59:24.57
Angular distance between the image centers 0.05 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 10:39:47.908 -17:59:20.14
Second-epoch second image center 10:39:45.894 -17:59:24.57
Angular distance between the image centers 0.00808 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits &> /tmp/tmp.wLusuK19x1
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits &> /tmp/tmp.iue3em4UAo
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits &> /tmp/tmp.WqRU0cy9iT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits &> /tmp/tmp.CZVp2tgKgG
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits and wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits and wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat
Found non-empty wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits and wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat
The reference image (wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits) and catalog (wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat) found
'wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat' -> 'wcsmag.cat'
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 5250 out of 7725 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.887548
a=0.000000 b=1.000000 c=22.887548
From vast_summary.log: estimated ref. image limiting mag.: -7.97
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.92
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.92
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
2.1 pix Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
2.5 pix fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits
2.4 pix fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits
Limiting magnitude estimates:
14.9 mag. Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
14.9 mag. Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
14.6 mag. fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits
14.6 mag. fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 11.8 (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.wLusuK19x1 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits' -> 'wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
WCS_IMAGE_NAME=wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
WCS-calibrated image found: wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
Checking if the catalog wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat corresponding to the image wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits alredy exist and is non-empty...
Catalog wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat corresponding to the image wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
WCS catalog name: wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=533, passed=7725
Got 7725 stars (including 7185 good ones) from the SExtractor catalog wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat
util/solve_plate_with_UCAC5 got 7725 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.26"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.26"
Estimated accuracy of the plate solution: 0.24"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits -region wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.iue3em4UAo (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits' -> 'wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
WCS_IMAGE_NAME=wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
WCS-calibrated image found: wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
Checking if the catalog wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat corresponding to the image wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits alredy exist and is non-empty...
Catalog wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat corresponding to the image wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
WCS catalog name: wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=531, passed=7630
Got 7630 stars (including 7093 good ones) from the SExtractor catalog wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat
util/solve_plate_with_UCAC5 got 7630 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.27"
Estimated accuracy of the plate solution: 0.24"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits -region wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.WqRU0cy9iT (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-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.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-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits
WCS_IMAGE_NAME=wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits
WCS-calibrated image found: wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits
Checking if the catalog wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits.cat corresponding to the image wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits.cat corresponding to the image wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.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-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits
WCS catalog name: wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=444, passed=6706
Got 6706 stars (including 6258 good ones) from the SExtractor catalog wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits.cat
util/solve_plate_with_UCAC5 got 6706 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.44"
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits -region wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.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.CZVp2tgKgG (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-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.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-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits
WCS_IMAGE_NAME=wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits
WCS-calibrated image found: wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits
Checking if the catalog wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits.cat corresponding to the image wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits.cat corresponding to the image wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.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-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits
WCS catalog name: wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=454, passed=6609
Got 6609 stars (including 6150 good ones) from the SExtractor catalog wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits.cat
util/solve_plate_with_UCAC5 got 6609 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.45"
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits -region wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.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-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits'
Saving fully-calibrated image wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits'
Saving fully-calibrated image wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits'
Saving fully-calibrated image wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits'
Preparing the HTML report for the field Hya-09-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20392.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 20385_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133
The candidate 20385_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133 did not pass the final checks
**** FOUND 10:56:51.90 -20:26:01.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20389_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133
The candidate 20389_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133 did not pass the final checks
**** FOUND 10:27:47.40 -19:52:51.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20392_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133
The candidate 20392_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133 did not pass the final checks
**** FOUND 11:01:26.19 -21:02:16.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 1.406 3551384006090056576 165.35879668740 -21.03759138398 12.2550 11.9379 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.406#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Hya-09-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits
SExtractor catalog cache: saved Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat to cache
SExtractor catalog cache: saved Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
Creating symlink local_wcs_cache/wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits exists and is non-empty
wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits exists and is non-empty
wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits exists and is non-empty
wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 10:39:59.375 -17:59:54.09
Second-epoch image center 10:39:47.908 -17:59:20.14
Angular distance between the image centers 0.05 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 10:39:59.375 -17:59:54.09
Second-epoch image center 10:39:45.894 -17:59:24.57
Angular distance between the image centers 0.05 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 10:39:47.908 -17:59:20.14
Second-epoch second image center 10:39:45.894 -17:59:24.57
Angular distance between the image centers 0.00808 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits &> /tmp/tmp.ob8q4vVpvl
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits &> /tmp/tmp.rfUxpij9fy
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits &> /tmp/tmp.w0f1EdPOJ3
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits &> /tmp/tmp.xM4pB5btBu
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits and wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits and wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat
Found non-empty wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits and wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat
The reference image (wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits) and catalog (wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat) found
'wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat' -> 'wcsmag.cat'
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 5627 out of 46060 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.755504
a=0.000000 b=1.000000 c=22.755504
From vast_summary.log: estimated ref. image limiting mag.: -7.73
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.03
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.03
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 43 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
2.0 pix Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
2.3 pix fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits
2.2 pix fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits
Limiting magnitude estimates:
15.0 mag. Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
15.0 mag. Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
14.8 mag. fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits
14.8 mag. fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 14.1 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.ob8q4vVpvl (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits' -> 'wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
WCS_IMAGE_NAME=wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
WCS-calibrated image found: wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
Checking if the catalog wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat corresponding to the image wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits alredy exist and is non-empty...
Catalog wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat corresponding to the image wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
WCS catalog name: wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=1888, passed=46057
Got 46057 stars (including 44088 good ones) from the SExtractor catalog wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat
util/solve_plate_with_UCAC5 got 46057 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.28"
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits -region wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.rfUxpij9fy (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits' -> 'wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
WCS_IMAGE_NAME=wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
WCS-calibrated image found: wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
Checking if the catalog wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat corresponding to the image wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits alredy exist and is non-empty...
Catalog wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat corresponding to the image wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
WCS catalog name: wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=1954, passed=46667
Got 46667 stars (including 44657 good ones) from the SExtractor catalog wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat
util/solve_plate_with_UCAC5 got 46667 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.29"
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits -region wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.w0f1EdPOJ3 (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-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.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-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits
WCS_IMAGE_NAME=wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits
WCS-calibrated image found: wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits
Checking if the catalog wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits.cat corresponding to the image wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits.cat corresponding to the image wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.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-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits
WCS catalog name: wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=1844, passed=39799
Got 39799 stars (including 37903 good ones) from the SExtractor catalog wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits.cat
util/solve_plate_with_UCAC5 got 39799 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.43"
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits -region wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.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.xM4pB5btBu (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-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.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-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits
WCS_IMAGE_NAME=wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits
WCS-calibrated image found: wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits
Checking if the catalog wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits.cat corresponding to the image wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits.cat corresponding to the image wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.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-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits
WCS catalog name: wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=1851, passed=40557
Got 40557 stars (including 38650 good ones) from the SExtractor catalog wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits.cat
util/solve_plate_with_UCAC5 got 40557 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.46"
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 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.46"
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Hya-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits -region wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.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-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.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-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/wcs_Hya-09-Q2b1x1_2025-12-23_04-04-07_20.00sec_-14.90C_LIGHT_0530.fits
Saving fully-calibrated image wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.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-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/wcs_Hya-09-Q2b1x1_2025-12-23_04-04-58_20.00sec_-14.90C_LIGHT_0531.fits
Saving fully-calibrated image wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.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-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-03-19_20.00sec_-15.00C_LIGHT_0132.fits
Saving fully-calibrated image wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.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-09-Q2b1x1_233549_TTUQ2b1x1_8631_SMoP0NtG/wcs_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133.fits
Preparing the HTML report for the field Hya-09-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out53703.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53708.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53713.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53716.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53724.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53730.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53732.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53736.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53841.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54052.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54064.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54084.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54094.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54106.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54110.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54118.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54120.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54128.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54134.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54151.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54172.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54208.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54249.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54267.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54298.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54346.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out53734.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54159.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 15s
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 53703_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133
The candidate 53703_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133 did not pass the final checks
**** FOUND 10:26:39.63 -13:44:29.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.24, MAG_FAINT_SEARCH_LIMIT=15.22)GAIADR2_OUTPUT=# 1.444 3754037266243885440 156.66552810599 -13.74158677177 14.2750 13.7931 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.444#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53708_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133
The candidate 53708_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133 did not pass the final checks
**** FOUND 10:14:20.44 -22:36:36.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.05, MAG_FAINT_SEARCH_LIMIT=15.03)GAIADR2_OUTPUT=# 1.259 5666154026364066944 153.58542633017 -22.60993987644 14.1503 13.6798 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.259#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53713_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133
The candidate 53713_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133 did not pass the final checks
**** FOUND 11:06:34.16 -14:21:31.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 0.907 3563299349176779776 166.64215235987 -14.35859687563 14.2170 13.6751 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.907#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53716_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133
The candidate 53716_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133 did not pass the final checks
**** FOUND 10:44:09.47 -16:50:36.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 1.072 3557106624811235712 161.03976821245 -16.84358298649 14.0523 13.4107 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.072#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53724_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133
The candidate 53724_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133 did not pass the final checks
**** FOUND 10:19:02.54 -17:54:33.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 0.799 5669905628757234688 154.76065714696 -17.90901162560 13.3214 12.6419 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.799#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53730_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133
The candidate 53730_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133 did not pass the final checks
**** FOUND 11:03:35.43 -13:03:58.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 0.589 3564463830774156160 165.89765310762 -13.06608880014 13.3281 12.8823 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.589#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53731_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133
The candidate 53731_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133 did not pass the final checks
**** FOUND 10:51:13.02 -20:21:18.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53732_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133
The candidate 53732_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133 did not pass the final checks
**** FOUND 10:56:43.73 -16:24:01.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 1.084 3556655687603878016 164.18189792897 -16.40045614396 13.6514 13.1195 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.084#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53733_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133
The candidate 53733_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133 did not pass the final checks
**** FOUND 11:04:27.76 -21:18:34.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53734_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133
Preparing report for the candidate 53734_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133
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Considering the candidate 53736_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133
The candidate 53736_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133 did not pass the final checks
**** FOUND 11:11:36.09 -23:00:14.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 5.168 3537985705288448896 167.89884670338 -23.00379662341 12.5161 11.8562 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.168#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53740_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133
The candidate 53740_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133 did not pass the final checks
**** FOUND 10:57:39.52 -12:57:41.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53743_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133
The candidate 53743_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133 did not pass the final checks
**** FOUND 10:59:13.25 -17:32:27.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53754_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133
The candidate 53754_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133 did not pass the final checks
**** FOUND 10:56:51.88 -20:26:01.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53801_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133
The candidate 53801_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133 did not pass the final checks
**** FOUND 10:44:04.78 -22:59:06.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53841_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133
The candidate 53841_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133 did not pass the final checks
**** FOUND 10:11:13.03 -18:57:25.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.83, MAG_FAINT_SEARCH_LIMIT=13.81)
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Considering the candidate 53849_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133
The candidate 53849_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133 did not pass the final checks
**** FOUND 10:56:40.95 -20:39:56.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53991_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133
The candidate 53991_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133 did not pass the final checks
**** FOUND 10:40:52.95 -22:48:40.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54052_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133
The candidate 54052_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133 did not pass the final checks
**** FOUND 11:05:16.00 -18:57:35.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 1.447 3552819113579093120 166.31707390471 -18.95960675251 14.0938 13.3348 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.447#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54062_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133
The candidate 54062_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133 did not pass the final checks
**** FOUND 11:08:46.68 -14:35:09.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54064_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133
The candidate 54064_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133 did not pass the final checks
**** FOUND 11:02:06.80 -19:37:21.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.28, MAG_FAINT_SEARCH_LIMIT=15.26)GAIADR2_OUTPUT=# 0.324 3552395389285927680 165.52823784481 -19.62260588787 14.3170 13.8098 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.324#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54084_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133
The candidate 54084_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133 did not pass the final checks
**** FOUND 11:00:50.26 -20:03:21.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 1.149 3552355325830968448 165.20952400491 -20.05569732222 14.3628 13.8319 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.149#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54094_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133
The candidate 54094_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133 did not pass the final checks
**** FOUND 10:52:29.27 -21:41:36.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.31, MAG_FAINT_SEARCH_LIMIT=15.29)GAIADR2_OUTPUT=# 1.658 3550551748804021632 163.12163995561 -21.69300823051 14.3484 13.8222 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.658#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54103_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133
The candidate 54103_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133 did not pass the final checks
**** FOUND 11:04:07.97 -14:13:27.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54106_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133
The candidate 54106_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133 did not pass the final checks
**** FOUND 10:49:58.67 -19:17:57.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.22, MAG_FAINT_SEARCH_LIMIT=15.20)GAIADR2_OUTPUT=# 2.484 3554152889902698368 162.49419689295 -19.30003322482 14.5687 14.0674 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.484#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54110_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133
The candidate 54110_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133 did not pass the final checks
**** FOUND 11:07:50.25 -13:23:39.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 0.690 3564217235227674240 166.95956631462 -13.39417600248 14.3877 13.8791 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.690#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54118_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133
The candidate 54118_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133 did not pass the final checks
**** FOUND 10:58:59.65 -21:30:58.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 0.685 3549862870409306752 164.74864502065 -21.51608572430 14.3690 13.9025 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.685#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54120_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133
The candidate 54120_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133 did not pass the final checks
**** FOUND 11:05:31.73 -17:55:01.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 0.511 3553045887852680832 166.38210051413 -17.91709650475 14.2652 13.7742 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.511#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54128_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133
The candidate 54128_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133 did not pass the final checks
**** FOUND 11:06:20.56 -18:01:54.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 2.264 3553028879782262528 166.58501494049 -18.03161588907 14.3790 13.6624 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.264#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54134_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133
The candidate 54134_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133 did not pass the final checks
**** FOUND 10:55:15.93 -21:32:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.42, MAG_FAINT_SEARCH_LIMIT=15.40)GAIADR2_OUTPUT=# 0.701 3549817996590917504 163.81658100231 -21.54793799845 14.3938 13.7836 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.701#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54144_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133
The candidate 54144_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133 did not pass the final checks
Rejecting candidate due to large distance (23.3") between the two second-epoch detections
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Considering the candidate 54147_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133
The candidate 54147_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133 did not pass the final checks
**** FOUND 10:59:53.87 -13:14:08.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54151_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133
The candidate 54151_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133 did not pass the final checks
**** FOUND 11:05:16.01 -17:20:00.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 3.042 3553268569020286592 166.31625736047 -17.33277273089 14.5515 14.0071 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.042#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54159_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133
Preparing report for the candidate 54159_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133
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Considering the candidate 54171_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133
The candidate 54171_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133 did not pass the final checks
**** FOUND 11:04:58.30 -13:18:45.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54172_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133
The candidate 54172_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133 did not pass the final checks
**** FOUND 11:06:29.97 -13:22:53.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.30, MAG_FAINT_SEARCH_LIMIT=15.28)GAIADR2_OUTPUT=# 1.145 3564209950963065600 166.62462438201 -13.38175981923 14.2796 13.7130 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.145#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54189_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133
The candidate 54189_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133 did not pass the final checks
**** FOUND 10:40:50.26 -13:26:26.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54208_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133
The candidate 54208_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133 did not pass the final checks
**** FOUND 11:01:19.78 -18:22:18.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)GAIADR2_OUTPUT=# 1.363 3553088115970668672 165.33208626200 -18.37145452062 14.4909 13.8517 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.363#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54249_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133
The candidate 54249_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133 did not pass the final checks
**** FOUND 11:01:27.63 -13:53:09.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)GAIADR2_OUTPUT=# 1.737 3564129068138995072 165.36527196509 -13.88551121302 14.2700 13.3962 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.737#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54267_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133
The candidate 54267_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133 did not pass the final checks
**** FOUND 11:05:19.06 -13:33:21.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)GAIADR2_OUTPUT=# 2.050 3564200295876573312 166.32940500091 -13.55543063681 14.4749 13.9879 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.050#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54298_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133
The candidate 54298_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133 did not pass the final checks
**** FOUND 10:57:07.05 -15:09:02.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.31, MAG_FAINT_SEARCH_LIMIT=15.29)GAIADR2_OUTPUT=# 1.696 3563556806696082560 164.27901345373 -15.15106650001 14.8292 14.4175 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.696#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54346_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133
The candidate 54346_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133 did not pass the final checks
**** FOUND 10:53:18.34 -13:08:06.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)GAIADR2_OUTPUT=# 1.666 3756239210077208064 163.32609773076 -13.13556532809 14.6085 14.1821 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.666#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 15170_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133
The candidate 15170_fd_Hya-09-Q2b1x1_2026-03-19_23-04-05_20.00sec_-14.90C_LIGHT_0133 did not pass the final checks