This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H
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 03.4524 2461347.9524 9.13 09:10:15.06 -02:22:15.8
232.76131 29.16954 galactic Hya Second-epoch detections are separated by 0.4" and 7.7 pix
The object was found in VSX 1" ASAS J091015-0222.3
Type: MISC
# Max. Min./Amp. JD0 Period
10.290 V Y 0.580 V 2452398.10000 79.100000000000 M4
The object was not found in astcheck.
Forced photometry on wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits at 09:10:15.06 -02:22:15.8: 10.31 +/- 0.00 detection
Forced photometry on wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits at 09:10:15.06 -02:22:15.8: 10.26 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.29 +/- 0.00
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
ASAS J091015-0222.3,2461347.9524,9.13,0.05,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
ASAS J091015-0222.3 20261103.4524 9.13CV 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 03.4524 2461347.9524 13.49 09:22:13.49 -06:46:04.6
238.84545 29.12275 galactic Hya Second-epoch detections are separated by 2.1" and 8.0 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 2 2 13.7 -0 0
Forced photometry on wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits at 09:22:13.49 -06:46:04.6: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits at 09:22:13.49 -06:46:04.6: 15.77 +/- 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,2461347.9524,13.49,0.05,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 20261103.4524 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461139.72300765 09.04.2026 05:20:57.861 /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits
First image: 2461139.72300765 09.04.2026 05:20:57.861 /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits
Last image: 2461347.95273591 03.11.2026 10:51:46.383 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 12
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.49
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): 8856
Objects passed selection criteria: 8851
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: 8366.75
Average stars matched: 8090 (96.6923 %)
Memory usage VmPeak: 234584 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 04:56:35 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: 2461139.72300765 09.04.2026 05:20:57.861 /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits
First image: 2461139.72300765 09.04.2026 05:20:57.861 /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits
Last image: 2461347.95273591 03.11.2026 10:51:46.383 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 23
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.19
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): 52763
Objects passed selection criteria: 52655
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: 45003.8
Average stars matched: 43185.8 (95.9603 %)
Memory usage VmPeak: 274380 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 04:57:29 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-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits
SExtractor catalog cache: saved Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits.cat to cache
SExtractor catalog cache: saved Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.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: 2461347.95207479
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits exists and is non-empty
wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits exists and is non-empty
wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits exists and is non-empty
wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits (1st reference image)
verification OK: wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits
Image size: 941.5'x626.9' 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: 09:25:53.268 -01:59:04.48 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-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits (1st new image)
verification OK: wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits
Image size: 941.1'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: 09:26:00.345 -01:59:56.73 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:25:53.268 -01:59:04.48
Second-epoch image center 09:26:00.345 -01:59:56.73
Angular distance between the image centers 0.0328 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits (2nd new image)
verification OK: wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits
Image size: 941.1'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: 09:25:57.885 -02:00:23.57 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:25:53.268 -01:59:04.48
Second-epoch image center 09:25:57.885 -02:00:23.57
Angular distance between the image centers 0.0292 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 09:26:00.345 -01:59:56.73
Second-epoch second image center 09:25:57.885 -02:00:23.57
Angular distance between the image centers 0.01267 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-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits &> /tmp/tmp.7aL1JGmD2b
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits &> /tmp/tmp.sIUf4QFi5u
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits &> /tmp/tmp.O9MFcbuCqW
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits &> /tmp/tmp.R0wjrcHQhU
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits and wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.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-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits and wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits.wcscat
Found non-empty wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits and wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits.wcscat
The reference image (wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits) and catalog (wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits.wcscat) found
'wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits.wcscat' -> 'wcsmag.cat'
Read 8667 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 133.2753 to 149.6594 deg, Dec -7.6871 to +3.7040 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 133.2753 to 149.6594 deg, Dec -7.6871 to 3.7040 deg
Loaded 7164 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): 5224 out of 5461 total matches.
Matched with Tycho-2 5461 out of 8667 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.749550
a=0.000000 b=1.000000 c=22.749550
From vast_summary.log: estimated ref. image limiting mag.: -7.49
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.26
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.26
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 8667 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 133.2753 to 149.6594 deg, Dec -7.6871 to +3.7040 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 133.2753 to 149.6594 deg, Dec -7.6871 to 3.7040 deg
Loaded 7164 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): 5224 out of 5461 total matches.
Matched with Tycho-2 5461 out of 8667 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits
Forced-photometry filter: calibrated wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits -> calib.txt_param_ref_wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits (aperture=6.3)
Read 9128 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 133.2207 to 149.5963 deg, Dec -7.7187 to +3.7039 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 133.2207 to 149.5963 deg, Dec -7.7187 to 3.7039 deg
Loaded 7204 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): 5263 out of 5506 total matches.
Matched with Tycho-2 5506 out of 9128 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits
Forced-photometry filter: calibrated wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits -> calib.txt_param_ref_wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits (aperture=6.2)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 12 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits
2.2 pix Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits
4.2 pix fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits
4.2 pix fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits
Limiting magnitude estimates:
15.3 mag. Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits
15.3 mag. Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits
14.6 mag. fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits
14.6 mag. fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 11.9 (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.7aL1JGmD2b (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-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits' -> 'wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.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-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits
WCS_IMAGE_NAME=wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits
WCS-calibrated image found: wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits
Checking if the catalog wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits.wcscat corresponding to the image wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits alredy exist and is non-empty...
Catalog wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits.wcscat corresponding to the image wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits
WCS catalog name: wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.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=631, bad_region=0, passed=8667
Got 8667 stars (including 8028 good ones) from the SExtractor catalog wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits.wcscat
util/solve_plate_with_UCAC5 got 8667 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 411 to 470 (Dec -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 4793 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4775 matched stars entering correct_measured_positions(), 4775 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4775 matched stars entering correct_measured_positions(), 8667 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 411 to 470 (Dec -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 4791 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4774 matched stars entering correct_measured_positions(), 8667 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4774 matched stars entering correct_measured_positions(), 8667 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4774 stars left (next iteration limit 5252)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits N_match=4774 sigma_overall_arcsec=0.359 sigma_q1_arcsec=0.400 sigma_q2_arcsec=0.424 sigma_q3_arcsec=0.320 sigma_q4_arcsec=0.327 n_q1=1026 n_q2=1151 n_q3=1182 n_q4=1415 worst_quadrant_to_overall_ratio=1.181
WCS_HEADER_DIAG: file=Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits selection=current_pairs N_selected=4774 N_valid=4774 bias_ra_arcsec=0.002 bias_dec_arcsec=-0.003 median_sep_arcsec=0.283 p95_sep_arcsec=0.908 n_q1=1026 n_q2=1151 n_q3=1182 n_q4=1415 occupied_cells_4x4=16/16
The image catalog is written to wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits -region wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.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.sIUf4QFi5u (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-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits' -> 'wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.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-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits
WCS_IMAGE_NAME=wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits
WCS-calibrated image found: wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits
Checking if the catalog wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits.wcscat corresponding to the image wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits alredy exist and is non-empty...
Catalog wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits.wcscat corresponding to the image wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits
WCS catalog name: wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.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=665, bad_region=0, passed=9128
Got 9128 stars (including 8453 good ones) from the SExtractor catalog wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits.wcscat
util/solve_plate_with_UCAC5 got 9128 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 411 to 470 (Dec -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 4803 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4782 matched stars entering correct_measured_positions(), 4783 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4782 matched stars entering correct_measured_positions(), 9128 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 411 to 470 (Dec -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 4803 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4782 matched stars entering correct_measured_positions(), 9128 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4782 matched stars entering correct_measured_positions(), 9128 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4782 stars left (next iteration limit 5260)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits N_match=4782 sigma_overall_arcsec=0.340 sigma_q1_arcsec=0.405 sigma_q2_arcsec=0.374 sigma_q3_arcsec=0.315 sigma_q4_arcsec=0.307 n_q1=999 n_q2=1145 n_q3=1181 n_q4=1457 worst_quadrant_to_overall_ratio=1.194
WCS_HEADER_DIAG: file=Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits selection=current_pairs N_selected=4782 N_valid=4782 bias_ra_arcsec=0.010 bias_dec_arcsec=0.009 median_sep_arcsec=0.275 p95_sep_arcsec=0.907 n_q1=999 n_q2=1145 n_q3=1181 n_q4=1457 occupied_cells_4x4=16/16
The image catalog is written to wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits -region wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.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.O9MFcbuCqW (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-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.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-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits
WCS_IMAGE_NAME=wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits
WCS-calibrated image found: wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits
Checking if the catalog wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits.wcscat corresponding to the image wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits.wcscat corresponding to the image wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.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-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits
WCS catalog name: wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.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=348, bad_region=1, passed=7924
Got 7924 stars (including 7571 good ones) from the SExtractor catalog wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits.wcscat
util/solve_plate_with_UCAC5 got 7924 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (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 0.010457 (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 412 to 469 (Dec -7.5 to 3.5)
Done reading UCAC5 zone files...
Matched 4783 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4760 matched stars entering correct_measured_positions(), 4760 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4760 matched stars entering correct_measured_positions(), 7924 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 412 to 469 (Dec -7.5 to 3.5)
Done reading UCAC5 zone files...
Matched 4784 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4760 matched stars entering correct_measured_positions(), 7924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4760 matched stars entering correct_measured_positions(), 7924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4760 stars left (next iteration limit 5236)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4760 robust_rms=12.826 arcsec worst_region_rms=27.886 arcsec outer_annulus_rms=27.886 arcsec
SIP_REFIT: SIP order 3 trial: matched=4760 robust_rms=0.466 arcsec worst_region_rms=0.748 arcsec outer_annulus_rms=0.748 arcsec
SIP_REFIT: SIP order 5 trial: matched=4760 robust_rms=0.339 arcsec worst_region_rms=0.541 arcsec outer_annulus_rms=0.541 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4760 robust_rms_before=1.247 arcsec robust_rms_before_corrected=0.343 arcsec robust_rms_after=0.339 arcsec worst_region_rms_before=0.551 worst_region_rms_after=0.541 outer_annulus_rms_before=1.710 outer_annulus_rms_after=0.541
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.551 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits worst_region_rms_kept=0.551 arcsec robust_rms_kept=0.343 arcsec matched=4760
WCS_QUALITY_DIAG: file=fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits N_match=4760 sigma_overall_arcsec=0.335 sigma_q1_arcsec=0.385 sigma_q2_arcsec=0.416 sigma_q3_arcsec=0.269 sigma_q4_arcsec=0.288 n_q1=1452 n_q2=1067 n_q3=1244 n_q4=997 worst_quadrant_to_overall_ratio=1.240
WCS_HEADER_DIAG: file=fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits selection=current_pairs N_selected=4760 N_valid=4760 bias_ra_arcsec=0.979 bias_dec_arcsec=0.104 median_sep_arcsec=1.152 p95_sep_arcsec=2.484 n_q1=1452 n_q2=1067 n_q3=1244 n_q4=997 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits -region wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.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.R0wjrcHQhU (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-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.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-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits
WCS_IMAGE_NAME=wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits
WCS-calibrated image found: wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits
Checking if the catalog wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits.wcscat corresponding to the image wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits.wcscat corresponding to the image wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.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-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits
WCS catalog name: wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.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=354, bad_region=0, passed=7932
Got 7932 stars (including 7574 good ones) from the SExtractor catalog wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits.wcscat
util/solve_plate_with_UCAC5 got 7932 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (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 0.010457 (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 412 to 469 (Dec -7.5 to 3.5)
Done reading UCAC5 zone files...
Matched 4782 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4758 matched stars entering correct_measured_positions(), 4759 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4758 matched stars entering correct_measured_positions(), 7932 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 412 to 469 (Dec -7.5 to 3.5)
Done reading UCAC5 zone files...
Matched 4783 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4758 matched stars entering correct_measured_positions(), 7932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4758 matched stars entering correct_measured_positions(), 7932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4758 stars left (next iteration limit 5233)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4758 robust_rms=12.851 arcsec worst_region_rms=27.731 arcsec outer_annulus_rms=27.731 arcsec
SIP_REFIT: SIP order 3 trial: matched=4758 robust_rms=0.454 arcsec worst_region_rms=0.767 arcsec outer_annulus_rms=0.767 arcsec
SIP_REFIT: SIP order 5 trial: matched=4758 robust_rms=0.332 arcsec worst_region_rms=0.549 arcsec outer_annulus_rms=0.549 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4758 robust_rms_before=1.243 arcsec robust_rms_before_corrected=0.346 arcsec robust_rms_after=0.332 arcsec worst_region_rms_before=0.552 worst_region_rms_after=0.549 outer_annulus_rms_before=1.672 outer_annulus_rms_after=0.549
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.552 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits worst_region_rms_kept=0.552 arcsec robust_rms_kept=0.346 arcsec matched=4758
WCS_QUALITY_DIAG: file=fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits N_match=4758 sigma_overall_arcsec=0.338 sigma_q1_arcsec=0.398 sigma_q2_arcsec=0.422 sigma_q3_arcsec=0.268 sigma_q4_arcsec=0.298 n_q1=1445 n_q2=1068 n_q3=1242 n_q4=1003 worst_quadrant_to_overall_ratio=1.247
WCS_HEADER_DIAG: file=fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits selection=current_pairs N_selected=4758 N_valid=4758 bias_ra_arcsec=0.959 bias_dec_arcsec=0.099 median_sep_arcsec=1.140 p95_sep_arcsec=2.555 n_q1=1445 n_q2=1068 n_q3=1242 n_q4=1003 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits -region wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.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-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits to local_wcs_cache/
'wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits' -> 'local_wcs_cache/wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits'
Saving the final (post-refit) wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits to local_wcs_cache/
'wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits' -> 'local_wcs_cache/wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits'
Saving the final (post-refit) wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits to local_wcs_cache/
'wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits' -> 'local_wcs_cache/wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits'
Saving the final (post-refit) wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits to local_wcs_cache/
'wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits' -> 'local_wcs_cache/wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits sigma_overall=0.359 worst_q_ratio=1.181
ref2=Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits sigma_overall=0.340 worst_q_ratio=1.194
new1=fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits sigma_overall=0.335 worst_q_ratio=1.240
new2=fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits sigma_overall=0.338 worst_q_ratio=1.247
reference average sigma_overall=0.3495 worst_q_ratio=1.1875
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117_astrometric_residuals.png (4774 matched stars from wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.32 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109_astrometric_residuals.png (4782 matched stars from wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.30 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517_astrometric_residuals.png (4760 matched stars from wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518_astrometric_residuals.png (4758 matched stars from wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.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-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits'
Saving fully-calibrated image wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits'
Preparing the HTML report for the field Hya-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits at 09:17:11.23 -00:05:12.1: 12.11 +/- 0.01 detection
Forced photometry on wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits at 09:19:43.78 -01:09:54.8: 12.12 +/- 0.01 detection
Forced photometry on wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits at 09:28:39.71 -00:05:42.8: 12.19 +/- 0.01 detection
Forced photometry on wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits at 09:04:43.32 +02:43:21.3: 12.34 +/- 0.02 detection
Forced photometry on wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits at 09:20:56.77 -01:22:44.0: 12.21 +/- 0.01 detection
Forced photometry on wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits at 09:21:39.34 +02:11:32.4: 12.21 +/- 0.01 detection
Forced photometry on wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits at 08:55:46.90 -05:33:22.2: 12.32 +/- 0.02 detection
Forced photometry on wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits at 09:01:02.94 -02:01:07.0: 12.32 +/- 0.02 detection
Forced photometry on wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits at 09:19:24.05 -01:06:39.9: 12.18 +/- 0.01 detection
Forced photometry on wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits at 09:17:11.23 -00:05:12.1: 12.16 +/- 0.01 detection
Forced photometry on wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits at 09:19:43.78 -01:09:54.8: 12.05 +/- 0.01 detection
Forced photometry on wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits at 09:21:39.34 +02:11:32.4: 12.22 +/- 0.01 detection
Forced photometry on wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits at 09:01:02.94 -02:01:07.0: 12.29 +/- 0.02 detection
Forced photometry on wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits at 09:28:39.71 -00:05:42.8: 12.20 +/- 0.01 detection
Forced photometry on wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits at 09:20:56.77 -01:22:44.0: 12.21 +/- 0.01 detection
Forced photometry on wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits at 09:19:24.05 -01:06:39.9: 12.16 +/- 0.01 detection
Forced photometry on wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits at 08:55:46.90 -05:33:22.2: 12.34 +/- 0.02 detection
Forced photometry on wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits at 09:04:43.32 +02:43:21.3: 12.29 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.14 +/- 0.01
Forced photometry reference-image weighted average: 12.08 +/- 0.01
Forced photometry reference-image weighted average: 12.30 +/- 0.01
Forced photometry filter REJECTED candidate at 09:17:11.23 -00:05:12.1: ref_mag=12.14 +/- 0.01 new_mean_mag=11.9956 delta=0.14 (need > 0.90)
Forced photometry reference-image weighted average: 12.21 +/- 0.01
Forced photometry reference-image weighted average: 12.21 +/- 0.01
Forced photometry reference-image weighted average: 12.19 +/- 0.01
Forced photometry reference-image weighted average: 12.33 +/- 0.02
Forced photometry filter REJECTED candidate at 09:01:02.94 -02:01:07.0: ref_mag=12.30 +/- 0.01 new_mean_mag=12.0252 delta=0.28 (need > 0.90)
Forced photometry reference-image weighted average: 12.17 +/- 0.01
Forced photometry filter REJECTED candidate at 09:21:39.34 +02:11:32.4: ref_mag=12.21 +/- 0.01 new_mean_mag=12.0940 delta=0.12 (need > 0.90)
Forced photometry reference-image weighted average: 12.31 +/- 0.01
Forced photometry filter REJECTED candidate at 09:20:56.77 -01:22:44.0: ref_mag=12.21 +/- 0.01 new_mean_mag=12.1007 delta=0.11 (need > 0.90)
Forced photometry filter REJECTED candidate at 09:19:43.78 -01:09:54.8: ref_mag=12.08 +/- 0.01 new_mean_mag=12.0241 delta=0.06 (need > 0.90)
Forced photometry filter REJECTED candidate at 09:28:39.71 -00:05:42.8: ref_mag=12.19 +/- 0.01 new_mean_mag=12.0184 delta=0.17 (need > 0.90)
Forced photometry filter REJECTED candidate at 08:55:46.90 -05:33:22.2: ref_mag=12.33 +/- 0.02 new_mean_mag=12.0901 delta=0.24 (need > 0.90)
Forced photometry filter REJECTED candidate at 09:19:24.05 -01:06:39.9: ref_mag=12.17 +/- 0.01 new_mean_mag=12.1002 delta=0.07 (need > 0.90)
Forced photometry filter REJECTED candidate at 09:04:43.32 +02:43:21.3: ref_mag=12.31 +/- 0.01 new_mean_mag=12.1103 delta=0.20 (need > 0.90)
Forced photometry on wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits at 09:10:15.06 -02:22:15.8: 10.31 +/- 0.00 detection
Forced photometry on wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits at 09:10:15.06 -02:22:15.8: 10.26 +/- 0.00 detection
Forced photometry reference-image weighted average: 10.29 +/- 0.00
Forced photometry filter KEPT candidate at 09:10:15.06 -02:22:15.8: ref_mag=10.29 +/- 0.00 new_mean_mag=9.1257 delta=1.16 (need > 0.90)
Adding exclusion_list_local.txt__out04448.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 4s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20900_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518
The candidate 20900_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20901_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518
The candidate 20901_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20902_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518
The candidate 20902_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20906_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518
The candidate 20906_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20908_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518
The candidate 20908_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20909_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518
The candidate 20909_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20910_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518
The candidate 20910_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20911_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518
The candidate 20911_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20915_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518
The candidate 20915_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08175_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518
The candidate 08175_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518 did not pass the final checks
**** FOUND 09:36:50.27 -05:49:42.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01418_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518
The candidate 01418_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518 did not pass the final checks
**** FOUND 09:06:12.86 +01:40:59.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04448_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518
Preparing report for the candidate 04448_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 5s
Prepared the HTML report for the field Hya-04-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 ####
09:10:15.06 -02:22:15.8
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-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits
SExtractor catalog cache: saved Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits.cat to cache
SExtractor catalog cache: saved Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits
Creating symlink local_wcs_cache/wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.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-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits exists and is non-empty
wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits exists and is non-empty
wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits exists and is non-empty
wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits (1st reference image)
verification OK: wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits
Image size: 941.5'x626.9' 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: 09:25:53.268 -01:59:04.48 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-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits (1st new image)
verification OK: wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits
Image size: 941.1'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: 09:26:00.345 -01:59:56.73 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:25:53.268 -01:59:04.48
Second-epoch image center 09:26:00.345 -01:59:56.73
Angular distance between the image centers 0.0328 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits (2nd new image)
verification OK: wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits
Image size: 941.1'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: 09:25:57.885 -02:00:23.57 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:25:53.268 -01:59:04.48
Second-epoch image center 09:25:57.885 -02:00:23.57
Angular distance between the image centers 0.0292 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 09:26:00.345 -01:59:56.73
Second-epoch second image center 09:25:57.885 -02:00:23.57
Angular distance between the image centers 0.01267 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-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits &> /tmp/tmp.Q2yKhNyBfN
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits &> /tmp/tmp.7I9MpUvhOl
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits &> /tmp/tmp.4PMtxtdLIH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits &> /tmp/tmp.hG3KYGJWwJ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits and wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.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-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits and wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits.wcscat
Found non-empty wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits and wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits.wcscat
The reference image (wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits) and catalog (wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits.wcscat) found
'wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits.wcscat' -> 'wcsmag.cat'
Read 56098 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 133.2495 to 149.6594 deg, Dec -7.7081 to +3.7641 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 133.2495 to 149.6594 deg, Dec -7.7081 to 3.7641 deg
Loaded 7232 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): 5038 out of 5658 total matches.
Matched with Tycho-2 5658 out of 56098 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.616500
a=0.000000 b=1.000000 c=22.616500
From vast_summary.log: estimated ref. image limiting mag.: -7.19
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.43
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.43
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 56098 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 133.2495 to 149.6594 deg, Dec -7.7081 to +3.7641 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 133.2495 to 149.6594 deg, Dec -7.7081 to 3.7641 deg
Loaded 7232 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): 5038 out of 5658 total matches.
Matched with Tycho-2 5658 out of 56098 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits
Forced-photometry filter: calibrated wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits -> calib.txt_param_ref_wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits (aperture=4.8)
Read 58569 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 133.2207 to 149.6387 deg, Dec -7.7456 to +3.7272 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 133.2207 to 149.6387 deg, Dec -7.7456 to 3.7272 deg
Loaded 7251 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): 5043 out of 5673 total matches.
Matched with Tycho-2 5673 out of 58569 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits
Forced-photometry filter: calibrated wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits -> calib.txt_param_ref_wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits (aperture=4.7)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 20 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits
2.0 pix Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits
3.9 pix fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits
3.8 pix fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits
Limiting magnitude estimates:
15.4 mag. Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits
15.5 mag. Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits
14.8 mag. fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits
14.8 mag. fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 13.9 (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.Q2yKhNyBfN (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-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits' -> 'wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.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-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits
WCS_IMAGE_NAME=wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits
WCS-calibrated image found: wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits
Checking if the catalog wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits.wcscat corresponding to the image wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits alredy exist and is non-empty...
Catalog wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits.wcscat corresponding to the image wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits
WCS catalog name: wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.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=26, blended=2885, bad_region=3, passed=56072
Got 56072 stars (including 53090 good ones) from the SExtractor catalog wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits.wcscat
util/solve_plate_with_UCAC5 got 56072 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 411 to 470 (Dec -7.7 to 3.8)
Done reading UCAC5 zone files...
Matched 4798 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4783 matched stars entering correct_measured_positions(), 4783 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4783 matched stars entering correct_measured_positions(), 56072 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 411 to 470 (Dec -7.7 to 3.8)
Done reading UCAC5 zone files...
Matched 4798 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4783 matched stars entering correct_measured_positions(), 56072 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4783 matched stars entering correct_measured_positions(), 56072 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4783 stars left (next iteration limit 5261)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.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-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits N_match=4783 sigma_overall_arcsec=0.338 sigma_q1_arcsec=0.377 sigma_q2_arcsec=0.393 sigma_q3_arcsec=0.306 sigma_q4_arcsec=0.317 n_q1=1027 n_q2=1161 n_q3=1175 n_q4=1420 worst_quadrant_to_overall_ratio=1.162
WCS_HEADER_DIAG: file=Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits selection=current_pairs N_selected=4783 N_valid=4783 bias_ra_arcsec=-0.011 bias_dec_arcsec=0.009 median_sep_arcsec=0.276 p95_sep_arcsec=0.896 n_q1=1027 n_q2=1161 n_q3=1175 n_q4=1420 occupied_cells_4x4=16/16
The image catalog is written to wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits -region wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.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.7I9MpUvhOl (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-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits' -> 'wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.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-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits
WCS_IMAGE_NAME=wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits
WCS-calibrated image found: wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits
Checking if the catalog wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits.wcscat corresponding to the image wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits alredy exist and is non-empty...
Catalog wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits.wcscat corresponding to the image wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits
WCS catalog name: wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.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=3114, bad_region=27, passed=58548
Got 58548 stars (including 55292 good ones) from the SExtractor catalog wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits.wcscat
util/solve_plate_with_UCAC5 got 58548 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 411 to 470 (Dec -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 4799 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4782 matched stars entering correct_measured_positions(), 4783 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4782 matched stars entering correct_measured_positions(), 58548 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 411 to 470 (Dec -7.7 to 3.7)
Done reading UCAC5 zone files...
Matched 4799 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4782 matched stars entering correct_measured_positions(), 58548 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4782 matched stars entering correct_measured_positions(), 58548 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4782 stars left (next iteration limit 5260)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.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-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits N_match=4782 sigma_overall_arcsec=0.323 sigma_q1_arcsec=0.380 sigma_q2_arcsec=0.358 sigma_q3_arcsec=0.301 sigma_q4_arcsec=0.284 n_q1=984 n_q2=1157 n_q3=1180 n_q4=1461 worst_quadrant_to_overall_ratio=1.177
WCS_HEADER_DIAG: file=Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits selection=current_pairs N_selected=4782 N_valid=4782 bias_ra_arcsec=-0.009 bias_dec_arcsec=0.015 median_sep_arcsec=0.269 p95_sep_arcsec=0.868 n_q1=984 n_q2=1157 n_q3=1180 n_q4=1461 occupied_cells_4x4=16/16
The image catalog is written to wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits -region wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.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.4PMtxtdLIH (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-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.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-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits
WCS_IMAGE_NAME=wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits
WCS-calibrated image found: wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits
Checking if the catalog wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits.wcscat corresponding to the image wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits.wcscat corresponding to the image wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.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-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits
WCS catalog name: wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.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=1538, bad_region=47, passed=33490
Got 33490 stars (including 31881 good ones) from the SExtractor catalog wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits.wcscat
util/solve_plate_with_UCAC5 got 33490 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (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 0.010457 (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 412 to 469 (Dec -7.5 to 3.5)
Done reading UCAC5 zone files...
Matched 4784 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4765 matched stars entering correct_measured_positions(), 4765 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4765 matched stars entering correct_measured_positions(), 33490 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
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 412 to 469 (Dec -7.5 to 3.5)
Done reading UCAC5 zone files...
Matched 4785 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4765 matched stars entering correct_measured_positions(), 33490 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4765 matched stars entering correct_measured_positions(), 33490 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4765 stars left (next iteration limit 5241)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.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=4765 robust_rms=12.921 arcsec worst_region_rms=28.383 arcsec outer_annulus_rms=28.383 arcsec
SIP_REFIT: SIP order 3 trial: matched=4765 robust_rms=0.468 arcsec worst_region_rms=0.759 arcsec outer_annulus_rms=0.759 arcsec
SIP_REFIT: SIP order 5 trial: matched=4765 robust_rms=0.337 arcsec worst_region_rms=0.541 arcsec outer_annulus_rms=0.541 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4765 robust_rms_before=1.255 arcsec robust_rms_before_corrected=0.341 arcsec robust_rms_after=0.337 arcsec worst_region_rms_before=0.576 worst_region_rms_after=0.541 outer_annulus_rms_before=1.719 outer_annulus_rms_after=0.541
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.576 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits worst_region_rms_kept=0.576 arcsec robust_rms_kept=0.341 arcsec matched=4765
WCS_QUALITY_DIAG: file=fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits N_match=4765 sigma_overall_arcsec=0.334 sigma_q1_arcsec=0.382 sigma_q2_arcsec=0.414 sigma_q3_arcsec=0.276 sigma_q4_arcsec=0.285 n_q1=1432 n_q2=1042 n_q3=1272 n_q4=1019 worst_quadrant_to_overall_ratio=1.240
WCS_HEADER_DIAG: file=fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits selection=current_pairs N_selected=4765 N_valid=4765 bias_ra_arcsec=0.987 bias_dec_arcsec=0.080 median_sep_arcsec=1.162 p95_sep_arcsec=2.521 n_q1=1432 n_q2=1042 n_q3=1272 n_q4=1019 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits -region wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.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.hG3KYGJWwJ (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-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.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-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits
WCS_IMAGE_NAME=wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits
WCS-calibrated image found: wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits
Checking if the catalog wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits.wcscat corresponding to the image wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits.wcscat corresponding to the image wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.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-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits
WCS catalog name: wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.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=6, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=1587, bad_region=47, passed=33594
Got 33594 stars (including 31930 good ones) from the SExtractor catalog wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits.wcscat
util/solve_plate_with_UCAC5 got 33594 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.1'
Seting catalog search parameters based on the expected field of view 941.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013071 (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 0.010457 (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 412 to 469 (Dec -7.5 to 3.5)
Done reading UCAC5 zone files...
Matched 4783 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4765 matched stars entering correct_measured_positions(), 4765 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4765 matched stars entering correct_measured_positions(), 33594 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
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 412 to 469 (Dec -7.5 to 3.5)
Done reading UCAC5 zone files...
Matched 4784 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4765 matched stars entering correct_measured_positions(), 33594 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4765 matched stars entering correct_measured_positions(), 33594 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4765 stars left (next iteration limit 5241)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.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=4765 robust_rms=12.836 arcsec worst_region_rms=28.421 arcsec outer_annulus_rms=28.421 arcsec
SIP_REFIT: SIP order 3 trial: matched=4765 robust_rms=0.458 arcsec worst_region_rms=0.779 arcsec outer_annulus_rms=0.779 arcsec
SIP_REFIT: SIP order 5 trial: matched=4765 robust_rms=0.329 arcsec worst_region_rms=0.550 arcsec outer_annulus_rms=0.550 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4765 robust_rms_before=1.249 arcsec robust_rms_before_corrected=0.340 arcsec robust_rms_after=0.329 arcsec worst_region_rms_before=0.552 worst_region_rms_after=0.550 outer_annulus_rms_before=1.683 outer_annulus_rms_after=0.550
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.552 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits worst_region_rms_kept=0.552 arcsec robust_rms_kept=0.340 arcsec matched=4765
WCS_QUALITY_DIAG: file=fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits N_match=4765 sigma_overall_arcsec=0.321 sigma_q1_arcsec=0.383 sigma_q2_arcsec=0.397 sigma_q3_arcsec=0.257 sigma_q4_arcsec=0.285 n_q1=1438 n_q2=1039 n_q3=1269 n_q4=1019 worst_quadrant_to_overall_ratio=1.239
WCS_HEADER_DIAG: file=fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits selection=current_pairs N_selected=4765 N_valid=4765 bias_ra_arcsec=0.966 bias_dec_arcsec=0.077 median_sep_arcsec=1.148 p95_sep_arcsec=2.560 n_q1=1438 n_q2=1039 n_q3=1269 n_q4=1019 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-11-03_CI_Hya-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits -region wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.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-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.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-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-50-49_20.00sec_-0.00C_LIGHTs_0517.fits
Saving fully-calibrated image wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.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-04-Q1b1x1_045231_TTUQ1b1x1_316546_JPsG0H1H/wcs_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518.fits
Preparing the HTML report for the field Hya-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits at 09:27:15.63 +02:54:39.8: 13.79 +/- 0.06 detection
Forced photometry on wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits at 08:55:29.02 -04:25:38.9: 13.61 +/- 0.06 detection
Forced photometry on wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits at 08:55:47.04 -02:23:35.0: 13.66 +/- 0.06 detection
Forced photometry on wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits at 09:18:00.16 -04:28:46.7: 13.77 +/- 0.05 detection
Forced photometry on wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits at 08:58:59.93 -06:32:37.5: 13.47 +/- 0.05 detection
Forced photometry on wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits at 09:02:01.43 +03:15:56.8: 13.38 +/- 0.05 detection
Forced photometry on wcs_Hya-04-Q1b1x1_2026-04-09_00-20-57_20.00sec_-4.90C_LIGHTs_0117.fits at 09:22:13.49 -06:46:04.6: 15.73 +/- 99.00 upperlimit
Forced photometry on wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits at 08:55:29.02 -04:25:38.9: 13.67 +/- 0.06 detection
Forced photometry on wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits at 08:55:47.04 -02:23:35.0: 13.72 +/- 0.06 detection
Forced photometry on wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits at 09:27:15.63 +02:54:39.8: 13.81 +/- 0.05 detection
Forced photometry on wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits at 09:18:00.16 -04:28:46.7: 13.80 +/- 0.05 detection
Forced photometry on wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits at 08:58:59.93 -06:32:37.5: 13.56 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.04
Forced photometry reference-image weighted average: 13.69 +/- 0.04
Forced photometry reference-image weighted average: 13.80 +/- 0.04
Forced photometry filter REJECTED candidate at 08:55:29.02 -04:25:38.9: ref_mag=13.64 +/- 0.04 new_mean_mag=13.5414 delta=0.10 (need > 0.90)
Forced photometry reference-image weighted average: 13.52 +/- 0.04
Forced photometry filter REJECTED candidate at 08:55:47.04 -02:23:35.0: ref_mag=13.69 +/- 0.04 new_mean_mag=13.9687 delta=-0.28 (need > 0.90)
Forced photometry reference-image weighted average: 13.79 +/- 0.04
Forced photometry filter REJECTED candidate at 09:27:15.63 +02:54:39.8: ref_mag=13.80 +/- 0.04 new_mean_mag=13.8099 delta=-0.01 (need > 0.90)
Forced photometry filter REJECTED candidate at 08:58:59.93 -06:32:37.5: ref_mag=13.52 +/- 0.04 new_mean_mag=13.7796 delta=-0.26 (need > 0.90)
Forced photometry filter REJECTED candidate at 09:18:00.16 -04:28:46.7: ref_mag=13.79 +/- 0.04 new_mean_mag=13.4654 delta=0.32 (need > 0.90)
Forced photometry on wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits at 09:02:01.43 +03:15:56.8: 13.59 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.04
Forced photometry filter REJECTED candidate at 09:02:01.43 +03:15:56.8: ref_mag=13.46 +/- 0.04 new_mean_mag=13.6157 delta=-0.15 (need > 0.90)
Forced photometry on wcs_Hya-04-Q1b1x1_2026-04-15_23-26-13_20.00sec_-4.90C_LIGHTs_0109.fits at 09:22:13.49 -06:46:04.6: 15.77 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out72559.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 54s
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 72048_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518
The candidate 72048_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518 did not pass the final checks
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Considering the candidate 72054_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518
The candidate 72054_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518 did not pass the final checks
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Considering the candidate 72068_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518
The candidate 72068_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518 did not pass the final checks
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Considering the candidate 72075_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518
The candidate 72075_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 72077_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518
The candidate 72077_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518 did not pass the final checks
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Considering the candidate 72080_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518
The candidate 72080_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518 did not pass the final checks
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Considering the candidate 72298_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518
The candidate 72298_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518 did not pass the final checks
**** FOUND 09:26:15.06 -01:28:52.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 72415_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518
The candidate 72415_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518 did not pass the final checks
**** FOUND 09:01:26.29 -02:31:18.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72422_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518
The candidate 72422_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518 did not pass the final checks
**** FOUND 09:53:40.95 +01:34:45.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72457_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518
The candidate 72457_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518 did not pass the final checks
**** FOUND 08:56:08.16 +01:40:05.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72470_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518
The candidate 72470_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518 did not pass the final checks
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Considering the candidate 72516_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518
The candidate 72516_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518 did not pass the final checks
**** FOUND 09:50:55.43 +00:49:12.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72559_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518
Preparing report for the candidate 72559_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518
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Considering the candidate 72574_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518
The candidate 72574_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518 did not pass the final checks
**** FOUND 09:35:27.07 -01:48:49.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72680_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518
The candidate 72680_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518 did not pass the final checks
**** FOUND 08:55:53.46 -02:59:19.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22481_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518
The candidate 22481_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518 did not pass the final checks
Rejecting candidate due to large distance (43.7") between the two second-epoch detections
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Considering the candidate 45695_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518
The candidate 45695_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518 did not pass the final checks
**** FOUND 09:36:50.27 -05:49:42.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 08985_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518
The candidate 08985_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518 did not pass the final checks
**** FOUND 09:06:12.86 +01:40:59.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25246_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518
The candidate 25246_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518 did not pass the final checks
**** FOUND 09:34:11.32 -01:53:12.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29578_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518
The candidate 29578_fd_Hya-04-Q1b1x1_2026-11-03_04-51-46_20.00sec_0.00C_LIGHTs_0518 did not pass the final checks