This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk
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 11 03.4661 2461347.9661 13.49 09:22:14.12 -06:46:13.9
238.84960 29.12332 galactic Hya Second-epoch detections are separated by 1.3" and 9.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.25 Phocaea 0 1 1 13.7 -0 0
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits at 09:22:14.12 -06:46:13.9: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits at 09:22:14.12 -06:46:13.9: 15.88 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461347.9661,13.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261103.4661 13.49CV 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
Mean magnitude and position on the discovery images:
2026 11 03.4661 2461347.9661 11.48 09:42:40.72 -15:09:02.8
249.83432 27.68514 galactic Hya Second-epoch detections are separated by 0.2" and 9.2 pix
The object was found in VSX 3" ASASSN-V J094240.87-150904.4
Type: L
# Max. Min./Amp. JD0 Period
12.440 V 13.430 V
The object was not found in astcheck.
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits at 09:42:40.72 -15:09:02.8: 12.66 +/- 0.03 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits at 09:42:40.72 -15:09:02.8: 12.64 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J094240.87-150904.4,2461347.9661,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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
ASASSN-V J094240.87-150904.4 20261103.4661 11.48CV 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461146.67400177 16.04.2026 04:10:23.753 /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits
First image: 2461146.67400177 16.04.2026 04:10:23.753 /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits
Last image: 2461347.96643727 03.11.2026 11:11:30.180 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 32
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.55
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 3
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
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 10058
Objects passed selection criteria: 10045
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: 9377.75
Average stars matched: 9160.75 (97.686 %)
Memory usage VmPeak: 235572 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Oct 15 15:05:03 CDT 2026
VaST build number 1.0rc89-241-g3eca6a38
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-15)
GNU bash, version 5.3.20(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Nov 3 05:17:05 CST 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461146.67400177 16.04.2026 04:10:23.753 /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits
First image: 2461146.67400177 16.04.2026 04:10:23.753 /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits
Last image: 2461347.96643727 03.11.2026 11:11:30.180 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 29
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.21
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: 16 seconds
Number of parallel threads: 3
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
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 62887
Objects passed selection criteria: 62750
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 52902.2
Average stars matched: 51215.2 (96.8111 %)
Memory usage VmPeak: 283576 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Oct 15 15:05:03 CDT 2026
VaST build number 1.0rc89-241-g3eca6a38
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-15)
GNU bash, version 5.3.20(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Nov 3 05:18:03 CST 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/TTUQ1b1x1/TTUQ1_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 --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits
SExtractor catalog cache: saved Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits.cat to cache
SExtractor catalog cache: saved Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.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-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits
Checking WCS cache directory local_wcs_cache
Checking 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: 2461347.96585123
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits exists and is non-empty
wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits exists and is non-empty
wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits exists and is non-empty
wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits (1st reference image)
verification OK: wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:25:43.554 -10:00:49.88 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits (1st new image)
verification OK: wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits
Image size: 941.0'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:25:57.258 -09:58:59.40 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:25:43.554 -10:00:49.88
Second-epoch image center 09:25:57.258 -09:58:59.40
Angular distance between the image centers 0.0641 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits (2nd new image)
verification OK: wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits
Image size: 941.0'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:25:54.534 -09:59:38.53 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:25:43.554 -10:00:49.88
Second-epoch image center 09:25:54.534 -09:59:38.53
Angular distance between the image centers 0.0492 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 09:25:57.258 -09:58:59.40
Second-epoch second image center 09:25:54.534 -09:59:38.53
Angular distance between the image centers 0.01559 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits &> /tmp/tmp.GWUokZ19PF
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits &> /tmp/tmp.sHrQlhKzE4
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits &> /tmp/tmp.LkmQappnnf
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits &> /tmp/tmp.LeRhza45Zt
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.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-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits and wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
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-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits and wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits.wcscat
Found non-empty wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits and wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits.wcscat
The reference image (wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits) and catalog (wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits.wcscat) found
'wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits.wcscat' -> 'wcsmag.cat'
Read 10001 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 133.0521 to 149.5826 deg, Dec -15.6737 to -4.1954 deg
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
Tycho-2 catalog search boundaries: RA 133.0521 to 149.5826 deg, Dec -15.6737 to -4.1954 deg
Loaded 8833 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 6200 out of 6476 total matches.
Matched with Tycho-2 6476 out of 10001 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.780350
a=0.000000 b=1.000000 c=22.780350
From vast_summary.log: estimated ref. image limiting mag.: -7.55
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.23
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.23
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 10001 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 133.0521 to 149.5826 deg, Dec -15.6737 to -4.1954 deg
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
Tycho-2 catalog search boundaries: RA 133.0521 to 149.5826 deg, Dec -15.6737 to -4.1954 deg
Loaded 8833 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 6200 out of 6476 total matches.
Matched with Tycho-2 6476 out of 10001 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits
Forced-photometry filter: calibrated wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits -> calib.txt_param_ref_wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits (aperture=6.2)
Read 10059 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 133.0521 to 149.6684 deg, Dec -15.6740 to -4.1954 deg
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
Tycho-2 catalog search boundaries: RA 133.0521 to 149.6684 deg, Dec -15.6740 to -4.1954 deg
Loaded 8867 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 6221 out of 6503 total matches.
Matched with Tycho-2 6503 out of 10059 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits
Forced-photometry filter: calibrated wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits -> calib.txt_param_ref_wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 32 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits
2.1 pix Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits
4.2 pix fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits
4.2 pix fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits
Limiting magnitude estimates:
15.2 mag. Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits
15.2 mag. Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits
14.5 mag. fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits
14.5 mag. fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits
All-image limiting magnitude estimate: 14.5 (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 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.GWUokZ19PF (6) ############
Parsing command line arguments...
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_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.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-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits' -> 'wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits
WCS_IMAGE_NAME=wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits
WCS-calibrated image found: wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits
Checking if the catalog wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits.wcscat corresponding to the image wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits alredy exist and is non-empty...
Catalog wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits.wcscat corresponding to the image wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits
WCS catalog name: wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=727, bad_region=0, passed=10001
Got 10001 stars (including 9264 good ones) from the SExtractor catalog wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits.wcscat
util/solve_plate_with_UCAC5 got 10001 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 431 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 4837 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4820 matched stars entering correct_measured_positions(), 4820 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4820 matched stars entering correct_measured_positions(), 10001 with non-zero local correction accuracy
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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 431 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 4836 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4819 matched stars entering correct_measured_positions(), 10001 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4819 matched stars entering correct_measured_positions(), 10001 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4819 stars left (next iteration limit 5302)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits N_match=4819 sigma_overall_arcsec=0.328 sigma_q1_arcsec=0.360 sigma_q2_arcsec=0.373 sigma_q3_arcsec=0.280 sigma_q4_arcsec=0.312 n_q1=1025 n_q2=1208 n_q3=1189 n_q4=1397 worst_quadrant_to_overall_ratio=1.138
WCS_HEADER_DIAG: file=Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits selection=current_pairs N_selected=4819 N_valid=4819 bias_ra_arcsec=-0.003 bias_dec_arcsec=0.001 median_sep_arcsec=0.265 p95_sep_arcsec=0.959 n_q1=1025 n_q2=1208 n_q3=1189 n_q4=1397 occupied_cells_4x4=16/16
The image catalog is written to wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits -region wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.sHrQlhKzE4 (6) ############
Parsing command line arguments...
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_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.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-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits' -> 'wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits
WCS_IMAGE_NAME=wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits
WCS-calibrated image found: wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits
Checking if the catalog wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits.wcscat corresponding to the image wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits alredy exist and is non-empty...
Catalog wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits.wcscat corresponding to the image wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits
WCS catalog name: wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=742, bad_region=0, passed=10059
Got 10059 stars (including 9308 good ones) from the SExtractor catalog wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits.wcscat
util/solve_plate_with_UCAC5 got 10059 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 431 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 4832 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4815 matched stars entering correct_measured_positions(), 4815 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4815 matched stars entering correct_measured_positions(), 10059 with non-zero local correction accuracy
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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 431 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 4832 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4814 matched stars entering correct_measured_positions(), 10059 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4814 matched stars entering correct_measured_positions(), 10059 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4814 stars left (next iteration limit 5296)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits N_match=4814 sigma_overall_arcsec=0.329 sigma_q1_arcsec=0.364 sigma_q2_arcsec=0.383 sigma_q3_arcsec=0.296 sigma_q4_arcsec=0.300 n_q1=1030 n_q2=1206 n_q3=1190 n_q4=1388 worst_quadrant_to_overall_ratio=1.166
WCS_HEADER_DIAG: file=Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits selection=current_pairs N_selected=4814 N_valid=4814 bias_ra_arcsec=-0.004 bias_dec_arcsec=-0.003 median_sep_arcsec=0.276 p95_sep_arcsec=0.947 n_q1=1030 n_q2=1206 n_q3=1190 n_q4=1388 occupied_cells_4x4=16/16
The image catalog is written to wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits -region wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.LkmQappnnf (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_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.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_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits
WCS_IMAGE_NAME=wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits
WCS-calibrated image found: wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits
Checking if the catalog wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits.wcscat corresponding to the image wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits.wcscat corresponding to the image wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits
WCS catalog name: wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=382, bad_region=0, passed=8834
Got 8834 stars (including 8446 good ones) from the SExtractor catalog wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits.wcscat
util/solve_plate_with_UCAC5 got 8834 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 429 (Dec -15.4 to -4.5)
Done reading UCAC5 zone files...
Matched 4844 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4823 matched stars entering correct_measured_positions(), 4823 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4823 matched stars entering correct_measured_positions(), 8834 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 429 (Dec -15.4 to -4.5)
Done reading UCAC5 zone files...
Matched 4844 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4823 matched stars entering correct_measured_positions(), 8834 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 4823 matched stars entering correct_measured_positions(), 8834 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4823 stars left (next iteration limit 5305)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4823 robust_rms=12.661 arcsec worst_region_rms=28.132 arcsec outer_annulus_rms=28.132 arcsec
SIP_REFIT: SIP order 3 trial: matched=4823 robust_rms=0.451 arcsec worst_region_rms=0.749 arcsec outer_annulus_rms=0.749 arcsec
SIP_REFIT: SIP order 5 trial: matched=4823 robust_rms=0.340 arcsec worst_region_rms=0.580 arcsec outer_annulus_rms=0.580 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4823 robust_rms_before=1.265 arcsec robust_rms_before_corrected=0.348 arcsec robust_rms_after=0.340 arcsec worst_region_rms_before=0.626 worst_region_rms_after=0.580 outer_annulus_rms_before=1.821 outer_annulus_rms_after=0.580
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.626 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits worst_region_rms_kept=0.626 arcsec robust_rms_kept=0.348 arcsec matched=4823
WCS_QUALITY_DIAG: file=fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits N_match=4823 sigma_overall_arcsec=0.335 sigma_q1_arcsec=0.411 sigma_q2_arcsec=0.394 sigma_q3_arcsec=0.280 sigma_q4_arcsec=0.275 n_q1=1391 n_q2=1079 n_q3=1333 n_q4=1020 worst_quadrant_to_overall_ratio=1.226
WCS_HEADER_DIAG: file=fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits selection=current_pairs N_selected=4823 N_valid=4823 bias_ra_arcsec=1.064 bias_dec_arcsec=-0.014 median_sep_arcsec=1.172 p95_sep_arcsec=2.685 n_q1=1391 n_q2=1079 n_q3=1333 n_q4=1020 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits -region wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.LeRhza45Zt (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_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.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_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits
WCS_IMAGE_NAME=wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits
WCS-calibrated image found: wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits
Checking if the catalog wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits.wcscat corresponding to the image wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits.wcscat corresponding to the image wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits
WCS catalog name: wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=383, bad_region=2, passed=8849
Got 8849 stars (including 8464 good ones) from the SExtractor catalog wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits.wcscat
util/solve_plate_with_UCAC5 got 8849 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 429 (Dec -15.4 to -4.4)
Done reading UCAC5 zone files...
Matched 4841 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4818 matched stars entering correct_measured_positions(), 4818 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4818 matched stars entering correct_measured_positions(), 8849 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 429 (Dec -15.4 to -4.4)
Done reading UCAC5 zone files...
Matched 4841 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4820 matched stars entering correct_measured_positions(), 8849 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 4820 matched stars entering correct_measured_positions(), 8849 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 4820 stars left (next iteration limit 5299)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4820 robust_rms=12.629 arcsec worst_region_rms=28.756 arcsec outer_annulus_rms=28.756 arcsec
SIP_REFIT: SIP order 3 trial: matched=4820 robust_rms=0.439 arcsec worst_region_rms=0.749 arcsec outer_annulus_rms=0.749 arcsec
SIP_REFIT: SIP order 5 trial: matched=4820 robust_rms=0.349 arcsec worst_region_rms=0.565 arcsec outer_annulus_rms=0.565 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4820 robust_rms_before=1.278 arcsec robust_rms_before_corrected=0.342 arcsec robust_rms_after=0.349 arcsec worst_region_rms_before=0.623 worst_region_rms_after=0.565 outer_annulus_rms_before=1.829 outer_annulus_rms_after=0.565
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.623 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits worst_region_rms_kept=0.623 arcsec robust_rms_kept=0.342 arcsec matched=4820
WCS_QUALITY_DIAG: file=fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits N_match=4820 sigma_overall_arcsec=0.327 sigma_q1_arcsec=0.403 sigma_q2_arcsec=0.398 sigma_q3_arcsec=0.272 sigma_q4_arcsec=0.275 n_q1=1396 n_q2=1067 n_q3=1333 n_q4=1024 worst_quadrant_to_overall_ratio=1.233
WCS_HEADER_DIAG: file=fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits selection=current_pairs N_selected=4820 N_valid=4820 bias_ra_arcsec=1.088 bias_dec_arcsec=0.026 median_sep_arcsec=1.181 p95_sep_arcsec=2.679 n_q1=1396 n_q2=1067 n_q3=1333 n_q4=1024 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits -region wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits to local_wcs_cache/
'wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits' -> 'local_wcs_cache/wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits'
Saving the final (post-refit) wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits to local_wcs_cache/
'wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits' -> 'local_wcs_cache/wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits'
Saving the final (post-refit) wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits to local_wcs_cache/
'wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits' -> 'local_wcs_cache/wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits'
Saving the final (post-refit) wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits to local_wcs_cache/
'wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits' -> 'local_wcs_cache/wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits sigma_overall=0.328 worst_q_ratio=1.138
ref2=Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits sigma_overall=0.329 worst_q_ratio=1.166
new1=fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits sigma_overall=0.335 worst_q_ratio=1.226
new2=fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits sigma_overall=0.327 worst_q_ratio=1.233
reference average sigma_overall=0.3285 worst_q_ratio=1.152
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094_astrometric_residuals.png (4819 matched stars from wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095_astrometric_residuals.png (4814 matched stars from wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.30 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535_astrometric_residuals.png (4823 matched stars from wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536_astrometric_residuals.png (4820 matched stars from wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits'
Saving fully-calibrated image wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits'
Preparing the HTML report for the field Hya-06-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits at 09:25:27.72 -05:59:30.2: 12.26 +/- 0.02 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits at 09:16:08.08 -05:17:29.1: 12.37 +/- 0.02 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits at 09:21:55.19 -07:59:59.0: 11.77 +/- 0.01 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits at 09:42:40.73 -15:09:03.4: 12.54 +/- 0.03 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits at 09:18:20.86 -06:51:56.7: 12.10 +/- 0.01 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits at 09:22:38.20 -08:33:13.0: 12.11 +/- 0.01 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits at 09:23:51.47 -08:02:36.0: 12.36 +/- 0.02 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits at 09:13:35.36 -10:02:19.2: 12.08 +/- 0.01 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits at 09:21:38.10 -09:42:13.1: 12.10 +/- 0.01 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits at 09:16:27.13 -08:46:58.1: 12.10 +/- 0.01 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits at 09:25:27.72 -05:59:30.2: 12.26 +/- 0.02 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits at 09:23:51.47 -08:02:36.0: 12.37 +/- 0.02 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits at 09:21:55.19 -07:59:59.0: 11.74 +/- 0.01 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits at 09:22:38.20 -08:33:13.0: 12.09 +/- 0.01 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits at 09:16:08.08 -05:17:29.1: 12.34 +/- 0.02 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits at 09:18:20.86 -06:51:56.7: 12.10 +/- 0.01 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits at 09:42:40.73 -15:09:03.4: 12.54 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.10 +/- 0.01
Forced photometry reference-image weighted average: 12.37 +/- 0.01
Forced photometry filter REJECTED candidate at 09:22:38.20 -08:33:13.0: ref_mag=12.10 +/- 0.01 new_mean_mag=11.9918 delta=0.11 (need > 0.90)
Forced photometry reference-image weighted average: 12.10 +/- 0.01
Forced photometry filter REJECTED candidate at 09:23:51.47 -08:02:36.0: ref_mag=12.37 +/- 0.01 new_mean_mag=11.7381 delta=0.63 (need > 0.90)
Forced photometry reference-image weighted average: 12.26 +/- 0.01
Forced photometry reference-image weighted average: 11.75 +/- 0.01
Forced photometry reference-image weighted average: 12.36 +/- 0.01
Forced photometry filter REJECTED candidate at 09:18:20.86 -06:51:56.7: ref_mag=12.10 +/- 0.01 new_mean_mag=11.9495 delta=0.15 (need > 0.90)
Forced photometry filter REJECTED candidate at 09:21:55.19 -07:59:59.0: ref_mag=11.75 +/- 0.01 new_mean_mag=11.6425 delta=0.11 (need > 0.90)
Forced photometry reference-image weighted average: 12.54 +/- 0.02
Forced photometry filter REJECTED candidate at 09:25:27.72 -05:59:30.2: ref_mag=12.26 +/- 0.01 new_mean_mag=11.9877 delta=0.27 (need > 0.90)
Forced photometry filter REJECTED candidate at 09:16:08.08 -05:17:29.1: ref_mag=12.36 +/- 0.01 new_mean_mag=11.9587 delta=0.40 (need > 0.90)
Forced photometry filter KEPT candidate at 09:42:40.73 -15:09:03.4: ref_mag=12.54 +/- 0.02 new_mean_mag=11.6336 delta=0.91 (need > 0.90)
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits at 09:13:35.36 -10:02:19.2: 12.09 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.08 +/- 0.01
Forced photometry filter REJECTED candidate at 09:13:35.36 -10:02:19.2: ref_mag=12.08 +/- 0.01 new_mean_mag=12.0056 delta=0.08 (need > 0.90)
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits at 09:16:27.13 -08:46:58.1: 12.12 +/- 0.01 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits at 09:21:38.10 -09:42:13.1: 12.12 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.11 +/- 0.01
Forced photometry reference-image weighted average: 12.11 +/- 0.01
Forced photometry filter REJECTED candidate at 09:16:27.13 -08:46:58.1: ref_mag=12.11 +/- 0.01 new_mean_mag=12.0141 delta=0.10 (need > 0.90)
Forced photometry filter REJECTED candidate at 09:21:38.10 -09:42:13.1: ref_mag=12.11 +/- 0.01 new_mean_mag=11.9846 delta=0.12 (need > 0.90)
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits at 09:13:06.26 -08:58:13.5: 12.19 +/- 0.01 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits at 09:24:33.82 -09:10:24.1: 12.14 +/- 0.01 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits at 08:55:46.93 -05:33:21.1: 12.36 +/- 0.02 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits at 09:23:44.57 -09:06:03.2: 12.12 +/- 0.01 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits at 09:11:41.02 -09:00:37.8: 12.25 +/- 0.01 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits at 09:00:10.67 -08:04:55.1: 12.43 +/- 0.02 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits at 09:22:42.01 -08:24:29.1: 12.13 +/- 0.01 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits at 09:11:45.86 -08:27:35.9: 12.29 +/- 0.02 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits at 09:13:06.26 -08:58:13.5: 12.17 +/- 0.01 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits at 09:23:44.57 -09:06:03.2: 12.10 +/- 0.01 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits at 09:24:33.82 -09:10:24.1: 12.12 +/- 0.01 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits at 09:11:41.02 -09:00:37.8: 12.24 +/- 0.02 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits at 09:00:10.67 -08:04:55.1: 12.36 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.11 +/- 0.01
Forced photometry reference-image weighted average: 12.18 +/- 0.01
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits at 08:55:46.93 -05:33:21.1: 12.31 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.25 +/- 0.01
Forced photometry filter REJECTED candidate at 09:23:44.57 -09:06:03.2: ref_mag=12.11 +/- 0.01 new_mean_mag=12.0246 delta=0.09 (need > 0.90)
Forced photometry reference-image weighted average: 12.13 +/- 0.01
Forced photometry reference-image weighted average: 12.39 +/- 0.01
Forced photometry filter REJECTED candidate at 09:13:06.26 -08:58:13.5: ref_mag=12.18 +/- 0.01 new_mean_mag=12.0592 delta=0.12 (need > 0.90)
Forced photometry filter REJECTED candidate at 09:00:10.67 -08:04:55.1: ref_mag=12.39 +/- 0.01 new_mean_mag=12.0903 delta=0.30 (need > 0.90)
Forced photometry filter REJECTED candidate at 09:11:41.02 -09:00:37.8: ref_mag=12.25 +/- 0.01 new_mean_mag=12.0915 delta=0.15 (need > 0.90)
Forced photometry filter REJECTED candidate at 09:24:33.82 -09:10:24.1: ref_mag=12.13 +/- 0.01 new_mean_mag=12.0411 delta=0.09 (need > 0.90)
Forced photometry reference-image weighted average: 12.33 +/- 0.02
Forced photometry filter REJECTED candidate at 08:55:46.93 -05:33:21.1: ref_mag=12.33 +/- 0.02 new_mean_mag=12.0125 delta=0.32 (need > 0.90)
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits at 09:11:45.86 -08:27:35.9: 12.27 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.28 +/- 0.01
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits at 09:22:42.01 -08:24:29.1: 12.12 +/- 0.01 detection
Forced photometry filter REJECTED candidate at 09:11:45.86 -08:27:35.9: ref_mag=12.28 +/- 0.01 new_mean_mag=12.0597 delta=0.22 (need > 0.90)
Forced photometry reference-image weighted average: 12.13 +/- 0.01
Forced photometry filter REJECTED candidate at 09:22:42.01 -08:24:29.1: ref_mag=12.13 +/- 0.01 new_mean_mag=12.0313 delta=0.10 (need > 0.90)
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits at 09:28:14.70 -05:30:38.2: 12.18 +/- 0.02 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits at 09:22:12.93 -08:31:43.5: 12.17 +/- 0.01 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits at 09:15:00.40 -09:31:46.0: 12.16 +/- 0.01 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits at 09:11:34.25 -08:50:25.0: 12.23 +/- 0.01 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits at 09:13:53.75 -09:31:24.5: 12.18 +/- 0.01 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits at 08:58:21.67 -06:40:57.4: 12.32 +/- 0.02 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits at 08:56:18.52 -08:48:33.7: 12.29 +/- 0.02 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits at 09:14:06.24 -09:18:09.4: 12.18 +/- 0.01 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits at 09:15:00.40 -09:31:46.0: 12.17 +/- 0.01 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits at 09:22:12.93 -08:31:43.5: 12.15 +/- 0.01 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits at 09:28:14.70 -05:30:38.2: 12.26 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.16 +/- 0.01
Forced photometry filter REJECTED candidate at 09:15:00.40 -09:31:46.0: ref_mag=12.16 +/- 0.01 new_mean_mag=12.0646 delta=0.10 (need > 0.90)
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits at 09:13:53.75 -09:31:24.5: 12.15 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.16 +/- 0.01
Forced photometry reference-image weighted average: 12.22 +/- 0.01
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits at 09:14:06.24 -09:18:09.4: 12.21 +/- 0.01 detection
Forced photometry filter REJECTED candidate at 09:22:12.93 -08:31:43.5: ref_mag=12.16 +/- 0.01 new_mean_mag=12.0674 delta=0.09 (need > 0.90)
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits at 08:56:18.52 -08:48:33.7: 12.25 +/- 0.02 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits at 08:58:21.67 -06:40:57.4: 12.36 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 09:28:14.70 -05:30:38.2: ref_mag=12.22 +/- 0.01 new_mean_mag=12.0708 delta=0.15 (need > 0.90)
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits at 09:11:34.25 -08:50:25.0: 12.21 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.16 +/- 0.01
Forced photometry reference-image weighted average: 12.19 +/- 0.01
Forced photometry filter REJECTED candidate at 09:13:53.75 -09:31:24.5: ref_mag=12.16 +/- 0.01 new_mean_mag=12.0124 delta=0.15 (need > 0.90)
Forced photometry filter REJECTED candidate at 09:14:06.24 -09:18:09.4: ref_mag=12.19 +/- 0.01 new_mean_mag=12.0452 delta=0.15 (need > 0.90)
Forced photometry reference-image weighted average: 12.27 +/- 0.01
Forced photometry reference-image weighted average: 12.34 +/- 0.01
Forced photometry reference-image weighted average: 12.22 +/- 0.01
Forced photometry filter REJECTED candidate at 08:56:18.52 -08:48:33.7: ref_mag=12.27 +/- 0.01 new_mean_mag=12.0824 delta=0.19 (need > 0.90)
Forced photometry filter REJECTED candidate at 08:58:21.67 -06:40:57.4: ref_mag=12.34 +/- 0.01 new_mean_mag=12.0602 delta=0.28 (need > 0.90)
Forced photometry filter REJECTED candidate at 09:11:34.25 -08:50:25.0: ref_mag=12.22 +/- 0.01 new_mean_mag=12.0588 delta=0.16 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out20547.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
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Considering the candidate 20547_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 20547_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
**** FOUND 09:42:40.73 -15:09:03.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#esa_tap#, MAG_MEAN=11.63, MAG_FAINT_SEARCH_LIMIT=12.61)GAIADR2_OUTPUT=# 2.220 5685743337841027968 145.67027619197 -15.15122714695 11.4165 10.1149 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.220#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20548_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 20548_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
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Considering the candidate 20549_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 20549_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
**** FOUND 09:56:32.56 -10:01:18.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20555_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 20555_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
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Considering the candidate 20569_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 20569_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
**** FOUND 09:03:07.82 -06:24:52.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20570_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 20570_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
**** FOUND 08:56:37.23 -07:50:22.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20579_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 20579_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
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Considering the candidate 20582_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 20582_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
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Considering the candidate 20586_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 20586_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
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Considering the candidate 20588_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 20588_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
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Considering the candidate 20589_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 20589_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
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Considering the candidate 20590_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 20590_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
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Considering the candidate 20594_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 20594_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
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Considering the candidate 20595_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 20595_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
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Considering the candidate 20601_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 20601_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
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Considering the candidate 20604_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 20604_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
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Considering the candidate 20606_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 20606_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
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Considering the candidate 20608_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 20608_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
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Considering the candidate 20609_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 20609_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
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Considering the candidate 20611_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 20611_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
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Considering the candidate 20612_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 20612_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
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Considering the candidate 20614_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 20614_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
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Considering the candidate 20615_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 20615_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
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Considering the candidate 20617_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 20617_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
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Considering the candidate 20618_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 20618_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
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Considering the candidate 20619_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 20619_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
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Considering the candidate 20621_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 20621_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
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Considering the candidate 20623_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 20623_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
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Considering the candidate 20624_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 20624_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
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Considering the candidate 00818_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 00818_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
**** FOUND 09:36:50.34 -05:49:44.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20184_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 20184_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
**** FOUND 09:04:02.64 -07:26:17.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 04261_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 04261_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
**** FOUND 08:55:40.09 -09:08:29.5 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 8s
Prepared the HTML report for the field Hya-06-Q1b1x1 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 --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits
SExtractor catalog cache: saved Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits.cat to cache
SExtractor catalog cache: saved Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.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-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits
Creating symlink local_wcs_cache/wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits
Checking 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-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits exists and is non-empty
wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits exists and is non-empty
wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits exists and is non-empty
wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits (1st reference image)
verification OK: wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:25:43.554 -10:00:49.88 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits (1st new image)
verification OK: wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits
Image size: 941.0'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:25:57.258 -09:58:59.40 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:25:43.554 -10:00:49.88
Second-epoch image center 09:25:57.258 -09:58:59.40
Angular distance between the image centers 0.0641 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits (2nd new image)
verification OK: wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits
Image size: 941.0'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:25:54.534 -09:59:38.53 J2000 4789.000 3195.000
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# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:25:43.554 -10:00:49.88
Second-epoch image center 09:25:54.534 -09:59:38.53
Angular distance between the image centers 0.0492 deg.
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# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 09:25:57.258 -09:58:59.40
Second-epoch second image center 09:25:54.534 -09:59:38.53
Angular distance between the image centers 0.01559 deg.
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Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits &> /tmp/tmp.xDQ2XGrTE7
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits &> /tmp/tmp.XnNgfyZeX5
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits &> /tmp/tmp.KnhXomVy2r
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits &> /tmp/tmp.Yin1pSQprT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.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-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits and wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
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-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits and wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits.wcscat
Found non-empty wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits and wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits.wcscat
The reference image (wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits) and catalog (wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits.wcscat) found
'wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits.wcscat' -> 'wcsmag.cat'
Read 68168 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 132.9922 to 149.6527 deg, Dec -15.6737 to -4.1954 deg
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
Tycho-2 catalog search boundaries: RA 132.9922 to 149.6527 deg, Dec -15.6737 to -4.1954 deg
Loaded 8899 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 6045 out of 6892 total matches.
Matched with Tycho-2 6892 out of 68168 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.634200
a=0.000000 b=1.000000 c=22.634200
From vast_summary.log: estimated ref. image limiting mag.: -7.21
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.42
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.42
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 68168 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 132.9922 to 149.6527 deg, Dec -15.6737 to -4.1954 deg
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
Tycho-2 catalog search boundaries: RA 132.9922 to 149.6527 deg, Dec -15.6737 to -4.1954 deg
Loaded 8899 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 6045 out of 6892 total matches.
Matched with Tycho-2 6892 out of 68168 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits
Forced-photometry filter: calibrated wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits -> calib.txt_param_ref_wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits (aperture=4.6)
Read 68122 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 132.9921 to 149.6684 deg, Dec -15.6809 to -4.1954 deg
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
Tycho-2 catalog search boundaries: RA 132.9921 to 149.6684 deg, Dec -15.6809 to -4.1954 deg
Loaded 8916 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 6046 out of 6893 total matches.
Matched with Tycho-2 6893 out of 68122 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits
Forced-photometry filter: calibrated wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits -> calib.txt_param_ref_wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits (aperture=4.6)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 27 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits
2.0 pix Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits
3.9 pix fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits
3.9 pix fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits
Limiting magnitude estimates:
15.4 mag. Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits
15.4 mag. Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits
14.7 mag. fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits
14.8 mag. fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 13.8 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.xDQ2XGrTE7 (6) ############
Parsing command line arguments...
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_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.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-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits' -> 'wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits
WCS_IMAGE_NAME=wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits
WCS-calibrated image found: wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits
Checking if the catalog wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits.wcscat corresponding to the image wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits alredy exist and is non-empty...
Catalog wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits.wcscat corresponding to the image wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits
WCS catalog name: wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=3914, bad_region=19, passed=68152
Got 68152 stars (including 64106 good ones) from the SExtractor catalog wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits.wcscat
util/solve_plate_with_UCAC5 got 68152 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 431 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 4833 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4819 matched stars entering correct_measured_positions(), 4819 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4819 matched stars entering correct_measured_positions(), 68152 with non-zero local correction accuracy
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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 431 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 4834 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4819 matched stars entering correct_measured_positions(), 68152 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4819 matched stars entering correct_measured_positions(), 68152 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4819 stars left (next iteration limit 5300)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits N_match=4819 sigma_overall_arcsec=0.322 sigma_q1_arcsec=0.351 sigma_q2_arcsec=0.350 sigma_q3_arcsec=0.279 sigma_q4_arcsec=0.324 n_q1=1023 n_q2=1204 n_q3=1178 n_q4=1414 worst_quadrant_to_overall_ratio=1.092
WCS_HEADER_DIAG: file=Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits selection=current_pairs N_selected=4819 N_valid=4819 bias_ra_arcsec=-0.015 bias_dec_arcsec=0.007 median_sep_arcsec=0.258 p95_sep_arcsec=0.966 n_q1=1023 n_q2=1204 n_q3=1178 n_q4=1414 occupied_cells_4x4=16/16
The image catalog is written to wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits -region wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.XnNgfyZeX5 (6) ############
Parsing command line arguments...
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_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.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-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits' -> 'wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits
WCS_IMAGE_NAME=wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits
WCS-calibrated image found: wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits
Checking if the catalog wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits.wcscat corresponding to the image wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits alredy exist and is non-empty...
Catalog wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits.wcscat corresponding to the image wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits
WCS catalog name: wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=21, blended=3852, bad_region=23, passed=68101
Got 68101 stars (including 64116 good ones) from the SExtractor catalog wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits.wcscat
util/solve_plate_with_UCAC5 got 68101 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 431 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 4830 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4818 matched stars entering correct_measured_positions(), 4818 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4818 matched stars entering correct_measured_positions(), 68101 with non-zero local correction accuracy
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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 371 to 431 (Dec -15.7 to -4.2)
Done reading UCAC5 zone files...
Matched 4830 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4818 matched stars entering correct_measured_positions(), 68101 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4818 matched stars entering correct_measured_positions(), 68101 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4818 stars left (next iteration limit 5299)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits N_match=4818 sigma_overall_arcsec=0.323 sigma_q1_arcsec=0.356 sigma_q2_arcsec=0.371 sigma_q3_arcsec=0.275 sigma_q4_arcsec=0.304 n_q1=1021 n_q2=1212 n_q3=1175 n_q4=1410 worst_quadrant_to_overall_ratio=1.149
WCS_HEADER_DIAG: file=Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits selection=current_pairs N_selected=4818 N_valid=4818 bias_ra_arcsec=-0.016 bias_dec_arcsec=0.001 median_sep_arcsec=0.269 p95_sep_arcsec=0.924 n_q1=1021 n_q2=1212 n_q3=1175 n_q4=1410 occupied_cells_4x4=16/16
The image catalog is written to wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits -region wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.KnhXomVy2r (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_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.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_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits
WCS_IMAGE_NAME=wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits
WCS-calibrated image found: wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits
Checking if the catalog wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits.wcscat corresponding to the image wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits.wcscat corresponding to the image wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits
WCS catalog name: wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=24, blended=2183, bad_region=46, passed=38732
Got 38732 stars (including 36468 good ones) from the SExtractor catalog wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits.wcscat
util/solve_plate_with_UCAC5 got 38732 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 429 (Dec -15.4 to -4.4)
Done reading UCAC5 zone files...
Matched 4839 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4823 matched stars entering correct_measured_positions(), 4823 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4823 matched stars entering correct_measured_positions(), 38732 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 373 to 429 (Dec -15.4 to -4.4)
Done reading UCAC5 zone files...
Matched 4839 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4824 matched stars entering correct_measured_positions(), 38732 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4824 matched stars entering correct_measured_positions(), 38732 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4824 stars left (next iteration limit 5305)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4824 robust_rms=12.722 arcsec worst_region_rms=27.923 arcsec outer_annulus_rms=27.923 arcsec
SIP_REFIT: SIP order 3 trial: matched=4824 robust_rms=0.457 arcsec worst_region_rms=0.755 arcsec outer_annulus_rms=0.755 arcsec
SIP_REFIT: SIP order 5 trial: matched=4824 robust_rms=0.343 arcsec worst_region_rms=0.568 arcsec outer_annulus_rms=0.568 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4824 robust_rms_before=1.277 arcsec robust_rms_before_corrected=0.343 arcsec robust_rms_after=0.343 arcsec worst_region_rms_before=0.606 worst_region_rms_after=0.568 outer_annulus_rms_before=1.811 outer_annulus_rms_after=0.568
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.606 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits worst_region_rms_kept=0.606 arcsec robust_rms_kept=0.343 arcsec matched=4824
WCS_QUALITY_DIAG: file=fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits N_match=4824 sigma_overall_arcsec=0.327 sigma_q1_arcsec=0.409 sigma_q2_arcsec=0.393 sigma_q3_arcsec=0.285 sigma_q4_arcsec=0.263 n_q1=1357 n_q2=1051 n_q3=1379 n_q4=1037 worst_quadrant_to_overall_ratio=1.251
WCS_HEADER_DIAG: file=fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits selection=current_pairs N_selected=4824 N_valid=4824 bias_ra_arcsec=1.071 bias_dec_arcsec=-0.028 median_sep_arcsec=1.182 p95_sep_arcsec=2.679 n_q1=1357 n_q2=1051 n_q3=1379 n_q4=1037 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits -region wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.Yin1pSQprT (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_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.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_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits
WCS_IMAGE_NAME=wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits
WCS-calibrated image found: wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits
Checking if the catalog wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits.wcscat corresponding to the image wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits.wcscat corresponding to the image wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits
WCS catalog name: wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=2062, bad_region=47, passed=38651
Got 38651 stars (including 36512 good ones) from the SExtractor catalog wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits.wcscat
util/solve_plate_with_UCAC5 got 38651 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 429 (Dec -15.4 to -4.4)
Done reading UCAC5 zone files...
Matched 4840 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4822 matched stars entering correct_measured_positions(), 4822 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4822 matched stars entering correct_measured_positions(), 38651 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 372 to 429 (Dec -15.4 to -4.4)
Done reading UCAC5 zone files...
Matched 4840 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4824 matched stars entering correct_measured_positions(), 38651 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4824 matched stars entering correct_measured_positions(), 38651 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4824 stars left (next iteration limit 5304)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4824 robust_rms=12.814 arcsec worst_region_rms=27.839 arcsec outer_annulus_rms=27.839 arcsec
SIP_REFIT: SIP order 3 trial: matched=4824 robust_rms=0.442 arcsec worst_region_rms=0.737 arcsec outer_annulus_rms=0.737 arcsec
SIP_REFIT: SIP order 5 trial: matched=4824 robust_rms=0.347 arcsec worst_region_rms=0.561 arcsec outer_annulus_rms=0.561 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4824 robust_rms_before=1.283 arcsec robust_rms_before_corrected=0.342 arcsec robust_rms_after=0.347 arcsec worst_region_rms_before=0.592 worst_region_rms_after=0.561 outer_annulus_rms_before=1.828 outer_annulus_rms_after=0.561
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.592 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits worst_region_rms_kept=0.592 arcsec robust_rms_kept=0.342 arcsec matched=4824
WCS_QUALITY_DIAG: file=fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits N_match=4824 sigma_overall_arcsec=0.327 sigma_q1_arcsec=0.404 sigma_q2_arcsec=0.387 sigma_q3_arcsec=0.270 sigma_q4_arcsec=0.270 n_q1=1358 n_q2=1046 n_q3=1376 n_q4=1044 worst_quadrant_to_overall_ratio=1.237
WCS_HEADER_DIAG: file=fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits selection=current_pairs N_selected=4824 N_valid=4824 bias_ra_arcsec=1.094 bias_dec_arcsec=0.005 median_sep_arcsec=1.187 p95_sep_arcsec=2.655 n_q1=1358 n_q2=1046 n_q3=1376 n_q4=1044 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits -region wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.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_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-10-39_20.00sec_-0.00C_LIGHTs_0535.fits
Saving fully-calibrated image wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.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_2026-11-03_CI_Hya-06-Q1b1x1_051216_TTUQ1b1x1_933307_yN7m3MBk/wcs_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536.fits
Preparing the HTML report for the field Hya-06-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits at 09:49:31.87 -14:35:30.1: 13.63 +/- 0.07 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits at 09:27:27.43 -14:30:05.5: 13.06 +/- 0.03 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits at 09:22:14.12 -06:46:13.9: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits at 09:46:35.51 -05:04:26.0: 99.00 +/- 99.00 edge
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits at 09:27:24.06 -07:57:08.8: 13.96 +/- 0.06 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits at 09:56:49.90 -14:41:47.3: 99.00 +/- 99.00 edge
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits at 09:20:17.64 -09:25:01.5: 13.83 +/- 0.05 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits at 09:35:27.37 -14:42:38.6: 12.77 +/- 0.04 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits at 09:46:35.51 -05:04:26.0: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 09:46:35.51 -05:04:26.0: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits at 09:27:27.43 -14:30:05.5: 12.99 +/- 0.03 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits at 09:56:49.90 -14:41:47.3: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 09:56:49.90 -14:41:47.3: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits at 09:22:14.12 -06:46:13.9: 15.88 +/- 99.00 upperlimit
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits at 09:49:31.87 -14:35:30.1: 13.46 +/- 0.06 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits at 09:20:17.64 -09:25:01.5: 13.86 +/- 0.06 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits at 09:27:24.06 -07:57:08.8: 13.87 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.02 +/- 0.02
Forced photometry filter REJECTED candidate at 09:27:27.43 -14:30:05.5: ref_mag=13.02 +/- 0.02 new_mean_mag=13.0058 delta=0.02 (need > 0.90)
Forced photometry reference-image weighted average: 13.53 +/- 0.04
Forced photometry reference-image weighted average: 13.85 +/- 0.04
Forced photometry reference-image weighted average: 13.92 +/- 0.04
Forced photometry filter REJECTED candidate at 09:49:31.87 -14:35:30.1: ref_mag=13.53 +/- 0.04 new_mean_mag=13.3589 delta=0.17 (need > 0.90)
Forced photometry filter REJECTED candidate at 09:20:17.64 -09:25:01.5: ref_mag=13.85 +/- 0.04 new_mean_mag=13.8469 delta=0.00 (need > 0.90)
Forced photometry filter REJECTED candidate at 09:27:24.06 -07:57:08.8: ref_mag=13.92 +/- 0.04 new_mean_mag=14.0347 delta=-0.12 (need > 0.90)
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits at 09:35:27.37 -14:42:38.6: 12.74 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.02
Forced photometry filter REJECTED candidate at 09:35:27.37 -14:42:38.6: ref_mag=12.75 +/- 0.02 new_mean_mag=13.2212 delta=-0.47 (need > 0.90)
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-10-23_20.00sec_-4.90C_LIGHTs_0094.fits at 09:42:40.72 -15:09:02.8: 12.66 +/- 0.03 detection
Forced photometry on wcs_Hya-06-Q1b1x1_2026-04-15_23-11-37_20.00sec_-5.00C_LIGHTs_0095.fits at 09:42:40.72 -15:09:02.8: 12.64 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.02
Forced photometry filter KEPT candidate at 09:42:40.72 -15:09:02.8: ref_mag=12.65 +/- 0.02 new_mean_mag=11.4820 delta=1.17 (need > 0.90)
Adding exclusion_list_local.txt__out42019.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out84022.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 29s
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 83506_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 83506_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
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Considering the candidate 83511_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 83511_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
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Considering the candidate 83530_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 83530_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
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Considering the candidate 83535_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 83535_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
**** FOUND 09:34:14.05 -05:05:55.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 83537_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 83537_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
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Considering the candidate 83544_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 83544_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
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Considering the candidate 83610_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 83610_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
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Considering the candidate 83952_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 83952_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
**** FOUND 09:13:20.43 -10:47:51.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 83979_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 83979_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
**** FOUND 09:02:05.13 -06:51:34.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 84022_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
Preparing report for the candidate 84022_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
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Considering the candidate 84025_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 84025_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
**** FOUND 09:16:38.20 -06:43:25.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 84057_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 84057_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
**** FOUND 09:43:07.90 -06:38:26.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 84092_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 84092_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
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Considering the candidate 84114_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 84114_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
**** FOUND 09:24:59.84 -13:16:17.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 84115_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 84115_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
**** FOUND 09:27:11.57 -05:04:55.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 84123_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 84123_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
**** FOUND 09:33:05.62 -10:06:04.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 84164_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 84164_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
**** FOUND 09:09:36.06 -09:56:59.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 84197_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 84197_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
**** FOUND 09:15:17.35 -08:28:21.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 44411_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 44411_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
**** FOUND 09:51:28.61 -14:50:49.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 42019_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
Preparing report for the candidate 42019_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
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Considering the candidate 33548_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 33548_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
**** FOUND 09:30:51.89 -10:16:08.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54270_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 54270_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
**** FOUND 09:42:09.88 -14:09:14.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 04894_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 04894_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
**** FOUND 09:36:50.34 -05:49:44.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 45181_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 45181_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
**** FOUND 09:22:53.92 -14:21:46.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29413_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 29413_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
**** FOUND 09:56:32.56 -10:01:18.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29885_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 29885_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks
**** FOUND 08:55:40.10 -09:08:29.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29391_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536
The candidate 29391_fd_Hya-06-Q1b1x1_2026-11-03_05-11-30_20.00sec_-0.00C_LIGHTs_0536 did not pass the final checks