This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC
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 10 19.3925 2461332.8925 10.71 09:35:22.50 +10:08:31.9
223.42751 40.91011 galactic Leo Second-epoch detections are separated by 0.5" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.6 Hebe 0 0 0 10.8 0 -0
Forced photometry on wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits at 09:35:22.50 +10:08:31.9: 15.68 +/- 99.00 upperlimit
Forced photometry on wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits at 09:35:22.50 +10:08:31.9: 15.70 +/- 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!
TCP 2026 10 19.3925* 09 35 22.50 +10 08 31.9 10.7 U Leo 9 0
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,2461332.8925,10.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261019.3925 10.71CV 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 10 19.3925 2461332.8925 13.05 09:15:15.32 +06:45:17.3
224.27022 34.92851 galactic Cnc Second-epoch detections are separated by 1.0" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.130 Elektra 0 1 1 13.4 -0 -0
Forced photometry on wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits at 09:15:15.32 +06:45:17.3: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits at 09:15:15.32 +06:45:17.3: 15.94 +/- 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,2461332.8925,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261019.3925 13.05CV 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: 2461136.69730958 06.04.2026 04:43:57.548 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
First image: 2461136.69730958 06.04.2026 04:43:57.548 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
Last image: 2461332.89277957 19.10.2026 09:25:26.155 /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.36
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 2 seconds
Number of parallel threads: 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): 7197
Objects passed selection criteria: 7168
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 5071.25
Average stars matched: 4639.25 (91.4814 %)
Memory usage VmPeak: 233196 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 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Oct 19 05:28:28 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461136.69730958 06.04.2026 04:43:57.548 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
First image: 2461136.69730958 06.04.2026 04:43:57.548 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
Last image: 2461332.89277957 19.10.2026 09:25:26.155 /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 24
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.03
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 12 seconds
Number of parallel threads: 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): 42426
Objects passed selection criteria: 42298
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 31421.2
Average stars matched: 28370.8 (90.2916 %)
Memory usage VmPeak: 261888 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 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Oct 19 05:29:25 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits
SExtractor catalog cache: saved Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits.cat to cache
SExtractor catalog cache: saved Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.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-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.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: 2461332.89217929
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-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits exists and is non-empty
wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits exists and is non-empty
wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits exists and is non-empty
wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits (1st reference image)
verification OK: wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
Image size: 937.5'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 09:25:48.169 +05:59:23.22 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits (1st new image)
verification OK: wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits
Image size: 940.5'x624.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 09:25:45.379 +05:57:06.93 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:25:48.169 +05:59:23.22
Second-epoch image center 09:25:45.379 +05:57:06.93
Angular distance between the image centers 0.0396 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits (2nd new image)
verification OK: wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits
Image size: 940.4'x624.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 09:25:42.426 +05:57:31.02 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:25:48.169 +05:59:23.22
Second-epoch image center 09:25:42.426 +05:57:31.02
Angular distance between the image centers 0.0392 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 09:25:45.379 +05:57:06.93
Second-epoch second image center 09:25:42.426 +05:57:31.02
Angular distance between the image centers 0.01395 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-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits &> /tmp/tmp.7wKtyAAyOT
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits &> /tmp/tmp.oBlVY54Yci
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits &> /tmp/tmp.VOXN3viQ59
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits &> /tmp/tmp.ar3My4x8Rx
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.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-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits and wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.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-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits and wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits.wcscat
Found non-empty wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits and wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits.wcscat
The reference image (wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits) and catalog (wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits.wcscat) found
'wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits.wcscat' -> 'wcsmag.cat'
Read 8779 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 133.4114 to 149.3504 deg, Dec +0.6257 to +11.2838 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 133.4114 to 149.3504 deg, Dec 0.6257 to 11.2838 deg
Loaded 5818 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): 4780 out of 4974 total matches.
Matched with Tycho-2 4974 out of 8779 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.770950
a=0.000000 b=1.000000 c=22.770950
From vast_summary.log: estimated ref. image limiting mag.: -7.36
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.41
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.41
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 8779 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 133.4114 to 149.3504 deg, Dec +0.6257 to +11.2838 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 133.4114 to 149.3504 deg, Dec 0.6257 to 11.2838 deg
Loaded 5818 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): 4780 out of 4974 total matches.
Matched with Tycho-2 4974 out of 8779 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
Forced-photometry filter: calibrated wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits -> calib.txt_param_ref_wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits (aperture=6.5)
Read 8775 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 133.4067 to 149.3394 deg, Dec +0.6451 to +11.2949 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 133.4067 to 149.3394 deg, Dec 0.6451 to 11.2949 deg
Loaded 5811 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): 4766 out of 4972 total matches.
Matched with Tycho-2 4972 out of 8775 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
Forced-photometry filter: calibrated wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits -> calib.txt_param_ref_wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits (aperture=6.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.5 pix Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
2.5 pix Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
2.4 pix fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits
2.4 pix fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits
Limiting magnitude estimates:
15.4 mag. Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
15.4 mag. Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
14.4 mag. fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits
14.5 mag. fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 11.5 (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.7wKtyAAyOT (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_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.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-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits' -> 'wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.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-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
WCS_IMAGE_NAME=wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
WCS-calibrated image found: wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
Checking if the catalog wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits.wcscat corresponding to the image wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits alredy exist and is non-empty...
Catalog wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits.wcscat corresponding to the image wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
WCS catalog name: wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=540, bad_region=2495, passed=8779
Got 8779 stars (including 5859 good ones) from the SExtractor catalog wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits.wcscat
util/solve_plate_with_UCAC5 got 8779 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 4748 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4733 matched stars entering correct_measured_positions(), 4733 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4733 matched stars entering correct_measured_positions(), 6747 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
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 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 4748 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4733 matched stars entering correct_measured_positions(), 6747 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 4733 matched stars entering correct_measured_positions(), 6747 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 4733 stars left (next iteration limit 5206)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits N_match=4733 sigma_overall_arcsec=0.397 sigma_q1_arcsec=0.388 sigma_q2_arcsec=0.404 sigma_q3_arcsec=0.405 sigma_q4_arcsec=0.387 n_q1=1308 n_q2=926 n_q3=1509 n_q4=990 worst_quadrant_to_overall_ratio=1.020
WCS_HEADER_DIAG: file=Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits selection=current_pairs N_selected=4733 N_valid=4733 bias_ra_arcsec=-0.008 bias_dec_arcsec=-0.010 median_sep_arcsec=0.322 p95_sep_arcsec=0.996 n_q1=1308 n_q2=926 n_q3=1509 n_q4=990 occupied_cells_4x4=16/16
The image catalog is written to wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits -region wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.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.oBlVY54Yci (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_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.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-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits' -> 'wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.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-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
WCS_IMAGE_NAME=wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
WCS-calibrated image found: wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
Checking if the catalog wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits.wcscat corresponding to the image wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits alredy exist and is non-empty...
Catalog wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits.wcscat corresponding to the image wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
WCS catalog name: wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=548, bad_region=2514, passed=8775
Got 8775 stars (including 5850 good ones) from the SExtractor catalog wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits.wcscat
util/solve_plate_with_UCAC5 got 8775 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 4753 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4735 matched stars entering correct_measured_positions(), 4735 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4735 matched stars entering correct_measured_positions(), 6738 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
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 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 4753 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4735 matched stars entering correct_measured_positions(), 6738 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 4735 matched stars entering correct_measured_positions(), 6738 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 4735 stars left (next iteration limit 5208)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits N_match=4735 sigma_overall_arcsec=0.415 sigma_q1_arcsec=0.414 sigma_q2_arcsec=0.421 sigma_q3_arcsec=0.419 sigma_q4_arcsec=0.408 n_q1=1324 n_q2=922 n_q3=1501 n_q4=988 worst_quadrant_to_overall_ratio=1.015
WCS_HEADER_DIAG: file=Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits selection=current_pairs N_selected=4735 N_valid=4735 bias_ra_arcsec=-0.002 bias_dec_arcsec=0.000 median_sep_arcsec=0.342 p95_sep_arcsec=1.026 n_q1=1324 n_q2=922 n_q3=1501 n_q4=988 occupied_cells_4x4=16/16
The image catalog is written to wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits -region wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.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.VOXN3viQ59 (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_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits
WCS_IMAGE_NAME=wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits
WCS-calibrated image found: wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits
Checking if the catalog wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits.wcscat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits.wcscat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits
WCS catalog name: wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=264, bad_region=698, passed=4629
Got 4629 stars (including 3706 good ones) from the SExtractor catalog wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits.wcscat
util/solve_plate_with_UCAC5 got 4629 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.5'
Seting catalog search parameters based on the expected field of view 940.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013063 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010450 (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 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 3517 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3504 matched stars entering correct_measured_positions(), 3505 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3504 matched stars entering correct_measured_positions(), 4073 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
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 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 3516 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3505 matched stars entering correct_measured_positions(), 4073 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 3505 matched stars entering correct_measured_positions(), 4073 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 3505 stars left (next iteration limit 3854)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3505 robust_rms=7.165 arcsec worst_region_rms=11.730 arcsec outer_annulus_rms=11.730 arcsec
SIP_REFIT: SIP order 3 trial: matched=3505 robust_rms=0.541 arcsec worst_region_rms=0.641 arcsec outer_annulus_rms=0.641 arcsec
SIP_REFIT: SIP order 5 trial: matched=3505 robust_rms=0.415 arcsec worst_region_rms=0.589 arcsec outer_annulus_rms=0.589 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3505 robust_rms_before=1.365 arcsec robust_rms_before_corrected=0.380 arcsec robust_rms_after=0.415 arcsec worst_region_rms_before=0.631 worst_region_rms_after=0.589 outer_annulus_rms_before=1.311 outer_annulus_rms_after=0.589
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.631 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits worst_region_rms_kept=0.631 arcsec robust_rms_kept=0.380 arcsec matched=3505
WCS_QUALITY_DIAG: file=fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits N_match=3505 sigma_overall_arcsec=0.381 sigma_q1_arcsec=0.399 sigma_q2_arcsec=0.360 sigma_q3_arcsec=0.377 sigma_q4_arcsec=0.415 n_q1=1300 n_q2=531 n_q3=1155 n_q4=519 worst_quadrant_to_overall_ratio=1.088
WCS_HEADER_DIAG: file=fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits selection=current_pairs N_selected=3505 N_valid=3505 bias_ra_arcsec=0.382 bias_dec_arcsec=0.438 median_sep_arcsec=1.210 p95_sep_arcsec=3.047 n_q1=1300 n_q2=531 n_q3=1155 n_q4=519 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits -region wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.ar3My4x8Rx (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_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.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_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits
WCS_IMAGE_NAME=wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits
WCS-calibrated image found: wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits
Checking if the catalog wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits.wcscat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits.wcscat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits
WCS catalog name: wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=253, bad_region=712, passed=4642
Got 4642 stars (including 3714 good ones) from the SExtractor catalog wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits.wcscat
util/solve_plate_with_UCAC5 got 4642 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.4'
Seting catalog search parameters based on the expected field of view 940.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013061 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010449 (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 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 3525 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3508 matched stars entering correct_measured_positions(), 3512 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3508 matched stars entering correct_measured_positions(), 4074 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
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 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 3524 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3510 matched stars entering correct_measured_positions(), 4074 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 3510 matched stars entering correct_measured_positions(), 4074 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 3510 stars left (next iteration limit 3858)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3510 robust_rms=7.259 arcsec worst_region_rms=11.410 arcsec outer_annulus_rms=11.410 arcsec
SIP_REFIT: SIP order 3 trial: matched=3510 robust_rms=0.565 arcsec worst_region_rms=0.683 arcsec outer_annulus_rms=0.683 arcsec
SIP_REFIT: SIP order 5 trial: matched=3510 robust_rms=0.406 arcsec worst_region_rms=0.588 arcsec outer_annulus_rms=0.588 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3510 robust_rms_before=1.403 arcsec robust_rms_before_corrected=0.381 arcsec robust_rms_after=0.406 arcsec worst_region_rms_before=0.648 worst_region_rms_after=0.588 outer_annulus_rms_before=1.312 outer_annulus_rms_after=0.588
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.648 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits worst_region_rms_kept=0.648 arcsec robust_rms_kept=0.381 arcsec matched=3510
WCS_QUALITY_DIAG: file=fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits N_match=3510 sigma_overall_arcsec=0.387 sigma_q1_arcsec=0.389 sigma_q2_arcsec=0.388 sigma_q3_arcsec=0.380 sigma_q4_arcsec=0.403 n_q1=1322 n_q2=536 n_q3=1137 n_q4=515 worst_quadrant_to_overall_ratio=1.041
WCS_HEADER_DIAG: file=fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits selection=current_pairs N_selected=3510 N_valid=3510 bias_ra_arcsec=0.391 bias_dec_arcsec=0.411 median_sep_arcsec=1.230 p95_sep_arcsec=2.908 n_q1=1322 n_q2=536 n_q3=1137 n_q4=515 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits -region wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.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-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits to local_wcs_cache/
'wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits' -> 'local_wcs_cache/wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits'
Saving the final (post-refit) wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits to local_wcs_cache/
'wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits' -> 'local_wcs_cache/wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits'
Saving the final (post-refit) wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits to local_wcs_cache/
'wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits' -> 'local_wcs_cache/wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits'
Saving the final (post-refit) wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits to local_wcs_cache/
'wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits' -> 'local_wcs_cache/wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits sigma_overall=0.397 worst_q_ratio=1.020
ref2=Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits sigma_overall=0.415 worst_q_ratio=1.015
new1=fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits sigma_overall=0.381 worst_q_ratio=1.088
new2=fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits sigma_overall=0.387 worst_q_ratio=1.041
reference average sigma_overall=0.406 worst_q_ratio=1.0175
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142_astrometric_residuals.png (4733 matched stars from wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143_astrometric_residuals.png (4735 matched stars from wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.37 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536_astrometric_residuals.png (3505 matched stars from wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537_astrometric_residuals.png (3510 matched stars from wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits'
Saving fully-calibrated image wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits'
Preparing the HTML report for the field Hya-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits at 09:35:22.50 +10:08:31.9: 15.68 +/- 99.00 upperlimit
Forced photometry on wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits at 09:35:22.50 +10:08:31.9: 15.70 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out20870.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20870_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537
Preparing report for the candidate 20870_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 7s
Prepared the HTML report for the field Hya-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
09:35:22.50 +10:08:31.9
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-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits
SExtractor catalog cache: saved Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits.cat to cache
SExtractor catalog cache: saved Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.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-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
Creating symlink local_wcs_cache/wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits
Creating symlink local_wcs_cache/wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.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-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits exists and is non-empty
wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits exists and is non-empty
wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits exists and is non-empty
wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits (1st reference image)
verification OK: wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
Image size: 937.5'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 09:25:48.169 +05:59:23.22 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits (1st new image)
verification OK: wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits
Image size: 940.5'x624.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 09:25:45.379 +05:57:06.93 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:25:48.169 +05:59:23.22
Second-epoch image center 09:25:45.379 +05:57:06.93
Angular distance between the image centers 0.0396 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits (2nd new image)
verification OK: wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits
Image size: 940.4'x624.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 09:25:42.426 +05:57:31.02 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:25:48.169 +05:59:23.22
Second-epoch image center 09:25:42.426 +05:57:31.02
Angular distance between the image centers 0.0392 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 09:25:45.379 +05:57:06.93
Second-epoch second image center 09:25:42.426 +05:57:31.02
Angular distance between the image centers 0.01395 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-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits &> /tmp/tmp.2EteZTV5jL
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits &> /tmp/tmp.cymEsrJUKI
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits &> /tmp/tmp.ErR5bUgkOg
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits &> /tmp/tmp.TI7v6zCRM0
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits
Calibrating the magnitude scale
Found non-empty wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.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-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits and wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.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-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits and wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits.wcscat
Found non-empty wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits and wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits.wcscat
The reference image (wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits) and catalog (wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits.wcscat) found
'wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits.wcscat' -> 'wcsmag.cat'
Read 49502 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 133.4115 to 149.3521 deg, Dec +0.6121 to +11.2883 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 133.4115 to 149.3521 deg, Dec 0.6121 to 11.2883 deg
Loaded 5828 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): 4553 out of 5057 total matches.
Matched with Tycho-2 5057 out of 49502 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.630400
a=0.000000 b=1.000000 c=22.630400
From vast_summary.log: estimated ref. image limiting mag.: -7.03
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.60
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.60
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 49502 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 133.4115 to 149.3521 deg, Dec +0.6121 to +11.2883 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 133.4115 to 149.3521 deg, Dec 0.6121 to 11.2883 deg
Loaded 5828 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): 4553 out of 5057 total matches.
Matched with Tycho-2 5057 out of 49502 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
Forced-photometry filter: calibrated wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits -> calib.txt_param_ref_wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits (aperture=4.9)
Read 49891 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 133.4067 to 149.3394 deg, Dec +0.6274 to +11.3006 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 133.4067 to 149.3394 deg, Dec 0.6274 to 11.3006 deg
Loaded 5822 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): 4546 out of 5059 total matches.
Matched with Tycho-2 5059 out of 49891 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
Forced-photometry filter: calibrated wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits -> calib.txt_param_ref_wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits (aperture=4.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 21 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
2.2 pix Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
2.3 pix fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits
2.3 pix fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits
Limiting magnitude estimates:
15.6 mag. Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
15.6 mag. Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
14.6 mag. fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits
14.6 mag. fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits
All-image limiting magnitude estimate: 14.6 (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.2EteZTV5jL (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_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.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-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits' -> 'wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.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-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
WCS_IMAGE_NAME=wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
WCS-calibrated image found: wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
Checking if the catalog wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits.wcscat corresponding to the image wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits alredy exist and is non-empty...
Catalog wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits.wcscat corresponding to the image wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits
WCS catalog name: wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=30, blended=2554, bad_region=11341, passed=49472
Got 49472 stars (including 36181 good ones) from the SExtractor catalog wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits.wcscat
util/solve_plate_with_UCAC5 got 49472 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 4747 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4736 matched stars entering correct_measured_positions(), 4736 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4736 matched stars entering correct_measured_positions(), 40961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
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 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 4747 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4736 matched stars entering correct_measured_positions(), 40961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4736 matched stars entering correct_measured_positions(), 40961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4736 stars left (next iteration limit 5209)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.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-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits N_match=4736 sigma_overall_arcsec=0.388 sigma_q1_arcsec=0.372 sigma_q2_arcsec=0.385 sigma_q3_arcsec=0.399 sigma_q4_arcsec=0.370 n_q1=1285 n_q2=944 n_q3=1498 n_q4=1009 worst_quadrant_to_overall_ratio=1.030
WCS_HEADER_DIAG: file=Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits selection=current_pairs N_selected=4736 N_valid=4736 bias_ra_arcsec=-0.044 bias_dec_arcsec=-0.007 median_sep_arcsec=0.311 p95_sep_arcsec=0.980 n_q1=1285 n_q2=944 n_q3=1498 n_q4=1009 occupied_cells_4x4=16/16
The image catalog is written to wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits -region wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.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.cymEsrJUKI (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_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.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-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits' -> 'wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.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-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
WCS_IMAGE_NAME=wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
WCS-calibrated image found: wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
Checking if the catalog wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits.wcscat corresponding to the image wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits alredy exist and is non-empty...
Catalog wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits.wcscat corresponding to the image wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits
WCS catalog name: wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=2614, bad_region=11386, passed=49870
Got 49870 stars (including 36533 good ones) from the SExtractor catalog wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits.wcscat
util/solve_plate_with_UCAC5 got 49870 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 4748 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4737 matched stars entering correct_measured_positions(), 4737 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4737 matched stars entering correct_measured_positions(), 41356 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
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 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 4748 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4737 matched stars entering correct_measured_positions(), 41356 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 4737 matched stars entering correct_measured_positions(), 41356 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 4737 stars left (next iteration limit 5210)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.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-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits N_match=4737 sigma_overall_arcsec=0.405 sigma_q1_arcsec=0.387 sigma_q2_arcsec=0.413 sigma_q3_arcsec=0.412 sigma_q4_arcsec=0.402 n_q1=1275 n_q2=961 n_q3=1486 n_q4=1015 worst_quadrant_to_overall_ratio=1.019
WCS_HEADER_DIAG: file=Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits selection=current_pairs N_selected=4737 N_valid=4737 bias_ra_arcsec=-0.035 bias_dec_arcsec=0.000 median_sep_arcsec=0.333 p95_sep_arcsec=1.032 n_q1=1275 n_q2=961 n_q3=1486 n_q4=1015 occupied_cells_4x4=16/16
The image catalog is written to wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits -region wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.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.ErR5bUgkOg (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_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits
WCS_IMAGE_NAME=wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits
WCS-calibrated image found: wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits
Checking if the catalog wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits.wcscat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits.wcscat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits
WCS catalog name: wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 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=5, blended=1011, bad_region=3121, passed=27951
Got 27951 stars (including 23969 good ones) from the SExtractor catalog wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits.wcscat
util/solve_plate_with_UCAC5 got 27951 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.5'
Seting catalog search parameters based on the expected field of view 940.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013063 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010450 (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 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 4740 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4719 matched stars entering correct_measured_positions(), 4720 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4719 matched stars entering correct_measured_positions(), 25604 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
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 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 4739 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4722 matched stars entering correct_measured_positions(), 25604 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 4722 matched stars entering correct_measured_positions(), 25604 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 4722 stars left (next iteration limit 5190)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4722 robust_rms=6.837 arcsec worst_region_rms=10.759 arcsec outer_annulus_rms=10.759 arcsec
SIP_REFIT: SIP order 3 trial: matched=4722 robust_rms=0.548 arcsec worst_region_rms=0.683 arcsec outer_annulus_rms=0.683 arcsec
SIP_REFIT: SIP order 5 trial: matched=4722 robust_rms=0.422 arcsec worst_region_rms=0.600 arcsec outer_annulus_rms=0.600 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4722 robust_rms_before=1.370 arcsec robust_rms_before_corrected=0.381 arcsec robust_rms_after=0.422 arcsec worst_region_rms_before=0.609 worst_region_rms_after=0.600 outer_annulus_rms_before=1.267 outer_annulus_rms_after=0.600
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.609 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits worst_region_rms_kept=0.609 arcsec robust_rms_kept=0.381 arcsec matched=4722
WCS_QUALITY_DIAG: file=fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits N_match=4722 sigma_overall_arcsec=0.377 sigma_q1_arcsec=0.387 sigma_q2_arcsec=0.367 sigma_q3_arcsec=0.373 sigma_q4_arcsec=0.390 n_q1=1742 n_q2=676 n_q3=1594 n_q4=710 worst_quadrant_to_overall_ratio=1.035
WCS_HEADER_DIAG: file=fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits selection=current_pairs N_selected=4722 N_valid=4722 bias_ra_arcsec=0.384 bias_dec_arcsec=0.441 median_sep_arcsec=1.212 p95_sep_arcsec=2.758 n_q1=1742 n_q2=676 n_q3=1594 n_q4=710 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits -region wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.TI7v6zCRM0 (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_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.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_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits
WCS_IMAGE_NAME=wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits
WCS-calibrated image found: wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits
Checking if the catalog wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits.wcscat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits alredy exist and is non-empty...
Catalog wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits.wcscat corresponding to the image wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits
WCS catalog name: wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=1, no_mag_err=0, low_SNR=3, blended=1069, bad_region=3195, passed=28299
Got 28299 stars (including 24194 good ones) from the SExtractor catalog wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits.wcscat
util/solve_plate_with_UCAC5 got 28299 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.4'
Seting catalog search parameters based on the expected field of view 940.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013061 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010449 (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 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 4740 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4720 matched stars entering correct_measured_positions(), 4721 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4720 matched stars entering correct_measured_positions(), 25887 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
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 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 4739 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4721 matched stars entering correct_measured_positions(), 25887 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 4721 matched stars entering correct_measured_positions(), 25887 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 4721 stars left (next iteration limit 5192)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.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=4721 robust_rms=6.957 arcsec worst_region_rms=10.815 arcsec outer_annulus_rms=10.815 arcsec
SIP_REFIT: SIP order 3 trial: matched=4721 robust_rms=0.569 arcsec worst_region_rms=0.697 arcsec outer_annulus_rms=0.697 arcsec
SIP_REFIT: SIP order 5 trial: matched=4721 robust_rms=0.415 arcsec worst_region_rms=0.599 arcsec outer_annulus_rms=0.599 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4721 robust_rms_before=1.406 arcsec robust_rms_before_corrected=0.380 arcsec robust_rms_after=0.415 arcsec worst_region_rms_before=0.629 worst_region_rms_after=0.599 outer_annulus_rms_before=1.292 outer_annulus_rms_after=0.599
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.629 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits worst_region_rms_kept=0.629 arcsec robust_rms_kept=0.380 arcsec matched=4721
WCS_QUALITY_DIAG: file=fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits N_match=4721 sigma_overall_arcsec=0.375 sigma_q1_arcsec=0.388 sigma_q2_arcsec=0.374 sigma_q3_arcsec=0.375 sigma_q4_arcsec=0.409 n_q1=1728 n_q2=680 n_q3=1608 n_q4=705 worst_quadrant_to_overall_ratio=1.092
WCS_HEADER_DIAG: file=fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits selection=current_pairs N_selected=4721 N_valid=4721 bias_ra_arcsec=0.403 bias_dec_arcsec=0.412 median_sep_arcsec=1.241 p95_sep_arcsec=2.758 n_q1=1728 n_q2=680 n_q3=1608 n_q4=705 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits -region wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.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-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-24-34_20.00sec_-0.00C_LIGHT_0536.fits
Saving fully-calibrated image wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.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_2026-10-19_CI_Hya-02-Q2b1x1_052611_TTUQ2b1x1_2624299_ROMuvhmC/wcs_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537.fits
Preparing the HTML report for the field Hya-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits at 09:29:26.97 +01:46:13.2: 12.78 +/- 0.02 detection
Forced photometry on wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits at 09:41:17.73 +09:00:36.0: 12.07 +/- 0.01 detection
Forced photometry on wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits at 09:15:15.32 +06:45:17.3: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Hya-02-Q2b1x1_2026-04-05_23-43-57_20.00sec_-5.00C_LIGHT_0142.fits at 09:19:53.31 +02:59:29.2: 13.66 +/- 0.05 detection
Forced photometry on wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits at 09:15:15.32 +06:45:17.3: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits at 09:29:26.97 +01:46:13.2: 12.84 +/- 0.02 detection
Forced photometry on wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits at 09:41:17.73 +09:00:36.0: 12.10 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.08 +/- 0.01
Forced photometry reference-image weighted average: 12.81 +/- 0.01
Forced photometry filter REJECTED candidate at 09:29:26.97 +01:46:13.2: ref_mag=12.81 +/- 0.01 new_mean_mag=12.9483 delta=-0.14 (need > 0.90)
Forced photometry filter REJECTED candidate at 09:41:17.73 +09:00:36.0: ref_mag=12.08 +/- 0.01 new_mean_mag=12.0110 delta=0.07 (need > 0.90)
Forced photometry on wcs_Hya-02-Q2b1x1_2026-04-05_23-44-56_20.00sec_-4.90C_LIGHT_0143.fits at 09:19:53.31 +02:59:29.2: 13.73 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.04
Forced photometry filter REJECTED candidate at 09:19:53.31 +02:59:29.2: ref_mag=13.69 +/- 0.04 new_mean_mag=13.5755 delta=0.12 (need > 0.90)
Adding exclusion_list_local.txt__out56654.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53088_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537
The candidate 53088_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537 did not pass the final checks
**** FOUND 09:09:45.84 +09:36:35.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53647_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537
The candidate 53647_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537 did not pass the final checks
**** FOUND 09:35:22.50 +10:08:32.2 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54765_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537
The candidate 54765_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537 did not pass the final checks
**** FOUND 09:40:58.89 +09:52:38.6 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54799_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537
The candidate 54799_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56529_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537
The candidate 56529_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537 did not pass the final checks
**** FOUND 09:37:18.98 +06:51:32.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56654_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537
Preparing report for the candidate 56654_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57041_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537
The candidate 57041_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57170_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537
The candidate 57170_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537 did not pass the final checks
**** FOUND 09:41:16.94 +04:41:34.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57853_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537
The candidate 57853_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537 did not pass the final checks
**** FOUND 09:25:28.06 +06:15:40.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57909_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537
The candidate 57909_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537 did not pass the final checks
**** FOUND 09:42:40.83 +08:07:14.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57949_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537
The candidate 57949_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537 did not pass the final checks
**** FOUND 09:41:02.11 +03:48:44.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57951_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537
The candidate 57951_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537 did not pass the final checks
**** FOUND 09:43:32.62 +06:13:02.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58193_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537
The candidate 58193_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537 did not pass the final checks
**** FOUND 09:37:17.54 +06:48:25.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58465_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537
The candidate 58465_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537 did not pass the final checks
**** FOUND 09:23:44.40 +05:13:58.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58551_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537
The candidate 58551_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537 did not pass the final checks
**** FOUND 09:28:35.68 +07:28:14.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58704_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537
The candidate 58704_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537 did not pass the final checks
**** FOUND 09:42:22.69 +07:24:15.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58732_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537
The candidate 58732_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58881_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537
The candidate 58881_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537 did not pass the final checks
**** FOUND 09:11:12.65 +09:47:37.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 59220_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537
The candidate 59220_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537 did not pass the final checks
**** FOUND 09:11:58.27 +03:07:51.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60370_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537
The candidate 60370_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537 did not pass the final checks
**** FOUND 09:35:31.76 +02:37:11.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09438_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537
The candidate 09438_fd_Hya-02-Q2b1x1_2026-10-19_04-25-26_20.00sec_-0.00C_LIGHT_0537 did not pass the final checks