This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ
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 08 16.3271 2461268.8271 13.85 03:37:45.57 +16:59:16.2
170.20581 -30.22926 galactic Tau Second-epoch detections are separated by 1.4" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.62 Erato -0 1 1 14.0 -0 0
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:37:45.57 +16:59:16.2: 16.18 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:37:45.57 +16:59:16.2: 16.22 +/- 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 08 16.3271* 03 37 45.57 +16 59 16.2 13.8 U Tau 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,2461268.8271,13.85,0.05,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 20260816.3271 13.85CV 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 08 16.3271 2461268.8271 14.01 03:18:54.08 +11:29:45.8
170.63683 -37.36324 galactic Ari Second-epoch detections are separated by 3.5" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1620 Geographos 4 -5 6 14.2 0 0
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:18:54.08 +11:29:45.8: 16.15 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:18:54.08 +11:29:45.8: 16.11 +/- 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 08 16.3271* 03 18 54.08 +11 29 45.8 14.0 U Ari 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,2461268.8271,14.01,0.05,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 20260816.3271 14.01CV 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: 2461049.67169814 09.01.2026 04:07:04.719 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
First image: 2461049.67169814 09.01.2026 04:07:04.719 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
Last image: 2461268.82733499 16.08.2026 07:51:11.743 /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.54
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 6372
Objects passed selection criteria: 6340
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 4247
Average stars matched: 3970.25 (93.4836 %)
Memory usage VmPeak: 232684 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Aug 14 19:27:11 CDT 2026
VaST build number 1.0rc89-191-g1c132b07
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-14)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Aug 16 03:20:30 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: 2461049.67169814 09.01.2026 04:07:04.719 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
First image: 2461049.67169814 09.01.2026 04:07:04.719 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
Last image: 2461268.82733499 16.08.2026 07:51:11.743 /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 13
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.21
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 10 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): 41022
Objects passed selection criteria: 40918
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 28580
Average stars matched: 26532.5 (92.8359 %)
Memory usage VmPeak: 262472 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Aug 14 19:27:11 CDT 2026
VaST build number 1.0rc89-191-g1c132b07
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-14)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Aug 16 03:21:09 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/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits
SExtractor catalog cache: saved Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.cat to cache
SExtractor catalog cache: saved Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.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/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461268.82682698
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_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits exists and is non-empty
wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits exists and is non-empty
wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits exists and is non-empty
wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits (1st reference image)
verification OK: wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 03:33:20.383 +13:59:53.59 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits (1st new image)
verification OK: wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits
Image size: 938.5'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 03:33:24.172 +14:02:45.20 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 03:33:20.383 +13:59:53.59
Second-epoch image center 03:33:24.172 +14:02:45.20
Angular distance between the image centers 0.0501 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits (2nd new image)
verification OK: wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits
Image size: 938.5'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 03:33:23.499 +14:02:15.90 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 03:33:20.383 +13:59:53.59
Second-epoch image center 03:33:23.499 +14:02:15.90
Angular distance between the image centers 0.0415 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 03:33:24.172 +14:02:45.20
Second-epoch second image center 03:33:23.499 +14:02:15.90
Angular distance between the image centers 0.00858 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/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits &> /tmp/tmp.IjPZ2SNwth
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits &> /tmp/tmp.JcitT6fCAp
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits &> /tmp/tmp.JjRjTdfIUm
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits &> /tmp/tmp.6FkPFi6K85
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.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_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits and wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.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_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits and wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat
Found non-empty wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits and wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat
The reference image (wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits) and catalog (wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat) found
'wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat' -> 'wcsmag.cat'
Read 7716 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 45.0636 to 61.6428 deg, Dec +8.6205 to +19.2872 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 45.0636 to 61.6428 deg, Dec 8.6205 to 19.2872 deg
Loaded 4361 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): 3534 out of 3742 total matches.
Matched with Tycho-2 3742 out of 7716 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.950750
a=0.000000 b=1.000000 c=22.950750
From vast_summary.log: estimated ref. image limiting mag.: -7.54
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 7716 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 45.0636 to 61.6428 deg, Dec +8.6205 to +19.2872 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 45.0636 to 61.6428 deg, Dec 8.6205 to 19.2872 deg
Loaded 4361 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): 3534 out of 3742 total matches.
Matched with Tycho-2 3742 out of 7716 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
Forced-photometry filter: calibrated wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits -> calib.txt_param_ref_wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits (aperture=6.0)
Read 7722 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 45.0650 to 61.6427 deg, Dec +8.6182 to +19.2791 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 45.0650 to 61.6427 deg, Dec 8.6182 to 19.2791 deg
Loaded 4354 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): 3534 out of 3736 total matches.
Matched with Tycho-2 3736 out of 7722 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
Forced-photometry filter: calibrated wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits -> calib.txt_param_ref_wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits (aperture=6.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
2.0 pix Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
2.3 pix fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits
2.3 pix fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits
Limiting magnitude estimates:
15.4 mag. Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
15.4 mag. Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
13.9 mag. fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits
13.9 mag. fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 11.3 (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.IjPZ2SNwth (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits' -> 'wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.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/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
WCS_IMAGE_NAME=wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
WCS-calibrated image found: wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
Checking if the catalog wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat corresponding to the image wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits alredy exist and is non-empty...
Catalog wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat corresponding to the image wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
WCS catalog name: wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.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=551, bad_region=1716, passed=7716
Got 7716 stars (including 5573 good ones) from the SExtractor catalog wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat
util/solve_plate_with_UCAC5 got 7716 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4903 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4894 matched stars entering correct_measured_positions(), 4894 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4894 matched stars entering correct_measured_positions(), 6339 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4903 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4894 matched stars entering correct_measured_positions(), 6339 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4894 matched stars entering correct_measured_positions(), 6339 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 4894 stars left (next iteration limit 5383)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits N_match=4894 sigma_overall_arcsec=0.317 sigma_q1_arcsec=0.399 sigma_q2_arcsec=0.313 sigma_q3_arcsec=0.271 sigma_q4_arcsec=0.268 n_q1=1724 n_q2=1005 n_q3=1514 n_q4=651 worst_quadrant_to_overall_ratio=1.261
The image catalog is written to wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits -region wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.JcitT6fCAp (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits' -> 'wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.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/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
WCS_IMAGE_NAME=wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
WCS-calibrated image found: wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
Checking if the catalog wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat corresponding to the image wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits alredy exist and is non-empty...
Catalog wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat corresponding to the image wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
WCS catalog name: wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.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=536, bad_region=1716, passed=7722
Got 7722 stars (including 5589 good ones) from the SExtractor catalog wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat
util/solve_plate_with_UCAC5 got 7722 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4905 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4897 matched stars entering correct_measured_positions(), 4897 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4897 matched stars entering correct_measured_positions(), 6342 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4905 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4898 matched stars entering correct_measured_positions(), 6342 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4898 matched stars entering correct_measured_positions(), 6342 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4898 stars left (next iteration limit 5386)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits N_match=4898 sigma_overall_arcsec=0.324 sigma_q1_arcsec=0.409 sigma_q2_arcsec=0.297 sigma_q3_arcsec=0.276 sigma_q4_arcsec=0.273 n_q1=1731 n_q2=1006 n_q3=1513 n_q4=648 worst_quadrant_to_overall_ratio=1.264
The image catalog is written to wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits -region wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.JjRjTdfIUm (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_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.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_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits
WCS_IMAGE_NAME=wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits
WCS-calibrated image found: wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits
Checking if the catalog wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits.wcscat corresponding to the image wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits.wcscat corresponding to the image wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits
WCS catalog name: wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.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=181, bad_region=671, passed=3200
Got 3200 stars (including 2369 good ones) from the SExtractor catalog wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits.wcscat
util/solve_plate_with_UCAC5 got 3200 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.5'
Seting catalog search parameters based on the expected field of view 938.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013035 (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 0.010428 (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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 2320 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2317 matched stars entering correct_measured_positions(), 2317 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2317 matched stars entering correct_measured_positions(), 2662 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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 2321 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2317 matched stars entering correct_measured_positions(), 2662 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 2317 matched stars entering correct_measured_positions(), 2662 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 2317 stars left (next iteration limit 2548)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=2317 robust_rms=7.108 arcsec worst_quadrant_rms=9.983 arcsec
SIP_REFIT: SIP order 3 trial: matched=2317 robust_rms=0.471 arcsec worst_quadrant_rms=0.511 arcsec
SIP_REFIT: SIP order 5 trial: matched=2317 robust_rms=0.399 arcsec worst_quadrant_rms=0.421 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=2317 robust_rms_before=1.030 arcsec robust_rms_before_corrected=0.404 arcsec robust_rms_after=0.399 arcsec worst_quadrant_rms_before=0.417 worst_quadrant_rms_after=0.421
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.417 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits N_match=2317 sigma_overall_arcsec=0.415 sigma_q1_arcsec=0.400 sigma_q2_arcsec=0.411 sigma_q3_arcsec=0.437 sigma_q4_arcsec=0.406 n_q1=626 n_q2=355 n_q3=831 n_q4=505 worst_quadrant_to_overall_ratio=1.053
The image catalog is written to wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits -region wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.6FkPFi6K85 (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_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.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_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits
WCS_IMAGE_NAME=wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits
WCS-calibrated image found: wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits
Checking if the catalog wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits.wcscat corresponding to the image wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits.wcscat corresponding to the image wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits
WCS catalog name: wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.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=174, bad_region=680, passed=3243
Got 3243 stars (including 2409 good ones) from the SExtractor catalog wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits.wcscat
util/solve_plate_with_UCAC5 got 3243 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.5'
Seting catalog search parameters based on the expected field of view 938.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013035 (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 0.010428 (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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 2357 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2354 matched stars entering correct_measured_positions(), 2354 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2354 matched stars entering correct_measured_positions(), 2691 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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 2358 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2354 matched stars entering correct_measured_positions(), 2691 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 2354 matched stars entering correct_measured_positions(), 2691 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 2354 stars left (next iteration limit 2589)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=2354 robust_rms=7.084 arcsec worst_quadrant_rms=10.037 arcsec
SIP_REFIT: SIP order 3 trial: matched=2354 robust_rms=0.482 arcsec worst_quadrant_rms=0.506 arcsec
SIP_REFIT: SIP order 5 trial: matched=2354 robust_rms=0.394 arcsec worst_quadrant_rms=0.441 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=2354 robust_rms_before=1.037 arcsec robust_rms_before_corrected=0.404 arcsec robust_rms_after=0.394 arcsec worst_quadrant_rms_before=0.424 worst_quadrant_rms_after=0.441
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.424 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits N_match=2354 sigma_overall_arcsec=0.413 sigma_q1_arcsec=0.427 sigma_q2_arcsec=0.389 sigma_q3_arcsec=0.430 sigma_q4_arcsec=0.409 n_q1=640 n_q2=367 n_q3=849 n_q4=498 worst_quadrant_to_overall_ratio=1.040
The image catalog is written to wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits -region wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Saving the final (post-refit) wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits to local_wcs_cache/
'wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits' -> 'local_wcs_cache/wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits'
Saving the final (post-refit) wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits to local_wcs_cache/
'wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits' -> 'local_wcs_cache/wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits'
Saving the final (post-refit) wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits to local_wcs_cache/
'wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits' -> 'local_wcs_cache/wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits'
Saving the final (post-refit) wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits to local_wcs_cache/
'wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits' -> 'local_wcs_cache/wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits sigma_overall=0.317 worst_q_ratio=1.261
ref2=Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits sigma_overall=0.324 worst_q_ratio=1.264
new1=fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits sigma_overall=0.415 worst_q_ratio=1.053
new2=fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits sigma_overall=0.413 worst_q_ratio=1.040
reference average sigma_overall=0.3205 worst_q_ratio=1.2625
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_astrometric_residuals.png (4894 matched stars from wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_astrometric_residuals.png (4898 matched stars from wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362_astrometric_residuals.png (2317 matched stars from wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.37 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363_astrometric_residuals.png (2354 matched stars from wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.37 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits'
Saving fully-calibrated image wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits'
Preparing the HTML report for the field Tau-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Tau-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits
SExtractor catalog cache: saved Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.cat to cache
SExtractor catalog cache: saved Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
Creating symlink local_wcs_cache/wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits exists and is non-empty
wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits exists and is non-empty
wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits exists and is non-empty
wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits (1st reference image)
verification OK: wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 03:33:20.383 +13:59:53.59 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits (1st new image)
verification OK: wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits
Image size: 938.5'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 03:33:24.172 +14:02:45.20 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 03:33:20.383 +13:59:53.59
Second-epoch image center 03:33:24.172 +14:02:45.20
Angular distance between the image centers 0.0501 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits (2nd new image)
verification OK: wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits
Image size: 938.5'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 03:33:23.499 +14:02:15.90 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 03:33:20.383 +13:59:53.59
Second-epoch image center 03:33:23.499 +14:02:15.90
Angular distance between the image centers 0.0415 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 03:33:24.172 +14:02:45.20
Second-epoch second image center 03:33:23.499 +14:02:15.90
Angular distance between the image centers 0.00858 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/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits &> /tmp/tmp.EIQ9rnd1iQ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits &> /tmp/tmp.2P41UpYuPZ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits &> /tmp/tmp.LxOYGPlkCP
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits &> /tmp/tmp.H0fUzHjxyK
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.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_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits and wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.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_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits and wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat
Found non-empty wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits and wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat
The reference image (wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits) and catalog (wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat) found
'wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat' -> 'wcsmag.cat'
Read 48584 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 45.0636 to 61.6458 deg, Dec +8.6191 to +19.2871 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 45.0636 to 61.6458 deg, Dec 8.6191 to 19.2871 deg
Loaded 4361 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): 3309 out of 3760 total matches.
Matched with Tycho-2 3760 out of 48584 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.817800
a=0.000000 b=1.000000 c=22.817800
From vast_summary.log: estimated ref. image limiting mag.: -7.21
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.61
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.61
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 48584 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 45.0636 to 61.6458 deg, Dec +8.6191 to +19.2871 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 45.0636 to 61.6458 deg, Dec 8.6191 to 19.2871 deg
Loaded 4361 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): 3309 out of 3760 total matches.
Matched with Tycho-2 3760 out of 48584 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
Forced-photometry filter: calibrated wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits -> calib.txt_param_ref_wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits (aperture=4.5)
Read 48560 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 45.0650 to 61.6548 deg, Dec +8.6183 to +19.2794 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 45.0650 to 61.6548 deg, Dec 8.6183 to 19.2794 deg
Loaded 4358 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): 3320 out of 3753 total matches.
Matched with Tycho-2 3753 out of 48560 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
Forced-photometry filter: calibrated wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits -> calib.txt_param_ref_wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits (aperture=4.6)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 10 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
1.9 pix Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
2.1 pix fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits
2.1 pix fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits
Limiting magnitude estimates:
15.6 mag. Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
15.6 mag. Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
14.2 mag. fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits
14.2 mag. fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 13.8 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.EIQ9rnd1iQ (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits' -> 'wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.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/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
WCS_IMAGE_NAME=wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
WCS-calibrated image found: wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
Checking if the catalog wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat corresponding to the image wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits alredy exist and is non-empty...
Catalog wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat corresponding to the image wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
WCS catalog name: wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.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=13, blended=2222, bad_region=8835, passed=48571
Got 48571 stars (including 37859 good ones) from the SExtractor catalog wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat
util/solve_plate_with_UCAC5 got 48571 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4899 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4893 matched stars entering correct_measured_positions(), 4893 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4893 matched stars entering correct_measured_positions(), 41607 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4899 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4893 matched stars entering correct_measured_positions(), 41607 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 4893 matched stars entering correct_measured_positions(), 41607 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4893 stars left (next iteration limit 5382)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.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_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits N_match=4893 sigma_overall_arcsec=0.310 sigma_q1_arcsec=0.385 sigma_q2_arcsec=0.297 sigma_q3_arcsec=0.269 sigma_q4_arcsec=0.268 n_q1=1704 n_q2=988 n_q3=1521 n_q4=680 worst_quadrant_to_overall_ratio=1.244
The image catalog is written to wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits -region wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.2P41UpYuPZ (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits' -> 'wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.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/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
WCS_IMAGE_NAME=wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
WCS-calibrated image found: wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
Checking if the catalog wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat corresponding to the image wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits alredy exist and is non-empty...
Catalog wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat corresponding to the image wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
WCS catalog name: wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.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=16, blended=2192, bad_region=8846, passed=48544
Got 48544 stars (including 37859 good ones) from the SExtractor catalog wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat
util/solve_plate_with_UCAC5 got 48544 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4897 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4890 matched stars entering correct_measured_positions(), 4890 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4890 matched stars entering correct_measured_positions(), 41566 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4897 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4891 matched stars entering correct_measured_positions(), 41566 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 4891 matched stars entering correct_measured_positions(), 41566 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4891 stars left (next iteration limit 5379)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.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_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits N_match=4891 sigma_overall_arcsec=0.310 sigma_q1_arcsec=0.392 sigma_q2_arcsec=0.285 sigma_q3_arcsec=0.263 sigma_q4_arcsec=0.271 n_q1=1699 n_q2=994 n_q3=1515 n_q4=683 worst_quadrant_to_overall_ratio=1.265
The image catalog is written to wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits -region wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.LxOYGPlkCP (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_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.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_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits
WCS_IMAGE_NAME=wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits
WCS-calibrated image found: wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits
Checking if the catalog wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits.wcscat corresponding to the image wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits.wcscat corresponding to the image wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits
WCS catalog name: wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.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=3, blended=612, bad_region=3036, passed=20844
Got 20844 stars (including 17334 good ones) from the SExtractor catalog wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits.wcscat
util/solve_plate_with_UCAC5 got 20844 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.5'
Seting catalog search parameters based on the expected field of view 938.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013035 (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 0.010428 (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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4895 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4883 matched stars entering correct_measured_positions(), 4883 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4883 matched stars entering correct_measured_positions(), 18596 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4894 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4883 matched stars entering correct_measured_positions(), 18596 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 4883 matched stars entering correct_measured_positions(), 18596 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 4883 stars left (next iteration limit 5371)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.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=4883 robust_rms=6.701 arcsec worst_quadrant_rms=10.021 arcsec
SIP_REFIT: SIP order 3 trial: matched=4883 robust_rms=0.516 arcsec worst_quadrant_rms=0.540 arcsec
SIP_REFIT: SIP order 5 trial: matched=4883 robust_rms=0.437 arcsec worst_quadrant_rms=0.484 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4883 robust_rms_before=1.032 arcsec robust_rms_before_corrected=0.429 arcsec robust_rms_after=0.437 arcsec worst_quadrant_rms_before=0.475 worst_quadrant_rms_after=0.484
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.475 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits N_match=4883 sigma_overall_arcsec=0.443 sigma_q1_arcsec=0.457 sigma_q2_arcsec=0.475 sigma_q3_arcsec=0.446 sigma_q4_arcsec=0.410 n_q1=1303 n_q2=668 n_q3=1864 n_q4=1048 worst_quadrant_to_overall_ratio=1.071
The image catalog is written to wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits -region wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.H0fUzHjxyK (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_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.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_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits
WCS_IMAGE_NAME=wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits
WCS-calibrated image found: wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits
Checking if the catalog wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits.wcscat corresponding to the image wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits.wcscat corresponding to the image wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits
WCS catalog name: wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.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=7, blended=591, bad_region=3036, passed=20757
Got 20757 stars (including 17245 good ones) from the SExtractor catalog wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits.wcscat
util/solve_plate_with_UCAC5 got 20757 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.5'
Seting catalog search parameters based on the expected field of view 938.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013035 (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 0.010428 (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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4900 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4892 matched stars entering correct_measured_positions(), 4892 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4892 matched stars entering correct_measured_positions(), 18538 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4898 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4890 matched stars entering correct_measured_positions(), 18538 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 4890 matched stars entering correct_measured_positions(), 18538 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 4890 stars left (next iteration limit 5381)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.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=4890 robust_rms=6.777 arcsec worst_quadrant_rms=10.204 arcsec
SIP_REFIT: SIP order 3 trial: matched=4890 robust_rms=0.510 arcsec worst_quadrant_rms=0.544 arcsec
SIP_REFIT: SIP order 5 trial: matched=4890 robust_rms=0.425 arcsec worst_quadrant_rms=0.492 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4890 robust_rms_before=1.040 arcsec robust_rms_before_corrected=0.418 arcsec robust_rms_after=0.425 arcsec worst_quadrant_rms_before=0.478 worst_quadrant_rms_after=0.492
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.478 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits N_match=4890 sigma_overall_arcsec=0.434 sigma_q1_arcsec=0.448 sigma_q2_arcsec=0.460 sigma_q3_arcsec=0.425 sigma_q4_arcsec=0.420 n_q1=1289 n_q2=680 n_q3=1871 n_q4=1050 worst_quadrant_to_overall_ratio=1.060
The image catalog is written to wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits -region wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
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_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.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_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-50-27_20.00sec_-0.00C_LIGHT_0362.fits
Saving fully-calibrated image wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.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_2026-08-16_CI_Tau-05-Q2b1x1_031640_TTUQ2b1x1_1646412_8EomdCdQ/wcs_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363.fits
Preparing the HTML report for the field Tau-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:18:54.08 +11:29:45.8: 16.15 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:27:14.86 +16:00:09.3: 11.71 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:37:45.57 +16:59:16.2: 16.18 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:23:30.49 +17:10:30.1: 14.51 +/- 0.09 detection
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:18:54.08 +11:29:45.8: 16.11 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:27:14.86 +16:00:09.3: 11.67 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:23:30.49 +17:10:30.1: 14.46 +/- 0.08 detection
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:37:45.57 +16:59:16.2: 16.22 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 11.69 +/- 0.00
Forced photometry reference-image weighted average: 14.48 +/- 0.06
Forced photometry filter REJECTED candidate at 03:27:14.86 +16:00:09.3: ref_mag=11.69 +/- 0.00 new_mean_mag=11.9081 delta=-0.21 (need > 0.90)
Forced photometry filter REJECTED candidate at 03:23:30.49 +17:10:30.1: ref_mag=14.48 +/- 0.06 new_mean_mag=14.1060 delta=0.37 (need > 0.90)
Adding exclusion_list_local.txt__out57234.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57596.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
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Considering the candidate 52890_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363
The candidate 52890_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363 did not pass the final checks
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Considering the candidate 55939_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363
The candidate 55939_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363 did not pass the final checks
**** FOUND 03:36:02.16 +16:29:19.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56213_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363
The candidate 56213_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363 did not pass the final checks
Rejecting candidate due to large distance (29.5") between the two second-epoch detections
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Considering the candidate 56274_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363
The candidate 56274_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363 did not pass the final checks
**** FOUND 03:49:22.11 +17:49:48.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56894_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363
The candidate 56894_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363 did not pass the final checks
**** FOUND 03:36:16.21 +17:49:42.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57145_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363
The candidate 57145_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363 did not pass the final checks
Rejecting candidate due to large distance (26.7") between the two second-epoch detections
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Considering the candidate 57234_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363
Preparing report for the candidate 57234_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363
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Considering the candidate 57596_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363
Preparing report for the candidate 57596_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363
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Considering the candidate 57603_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363
The candidate 57603_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363 did not pass the final checks
Rejecting candidate due to large distance (26.3") between the two second-epoch detections
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Considering the candidate 57681_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363
The candidate 57681_fd_Tau-05-Q2b1x1_2026-08-16_02-51-11_20.00sec_-0.00C_LIGHT_0363 did not pass the final checks