This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n
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 18.3657 2461270.8657 13.65 04:39:53.18 +17:06:06.4
181.09415 -19.13541 galactic Tau Second-epoch detections are separated by 1.3" and 9.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.53 Kalypso -0 1 1 13.6 -0 0
Forced photometry on wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits at 04:39:53.18 +17:06:06.4: 16.24 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits at 04:39:53.18 +17:06:06.4: 16.15 +/- 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 18.3657* 04 39 53.18 +17 06 06.4 13.7 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,2461270.8657,13.65,0.05,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 20260818.3657 13.65CV 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 18.3657 2461270.8657 13.96 04:38:25.96 +16:18:51.3
181.52947 -19.89238 galactic Tau Second-epoch detections are separated by 0.9" and 10.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.670 Ottegebe 1 -0 1 14.3 0 0
Forced photometry on wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits at 04:38:25.96 +16:18:51.3: 16.23 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits at 04:38:25.96 +16:18:51.3: 16.17 +/- 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 18.3657* 04 38 25.96 +16 18 51.3 14.0 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,2461270.8657,13.96,0.05,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 20260818.3657 13.96CV 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: 2461049.68246666 09.01.2026 04:22:35.119 /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
First image: 2461049.68246666 09.01.2026 04:22:35.119 /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
Last image: 2461270.86617343 18.08.2026 08:47:07.384 /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.54
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): 7600
Objects passed selection criteria: 7577
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 5558
Average stars matched: 5207.5 (93.6938 %)
Memory usage VmPeak: 233612 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 Tue Aug 18 04:02:28 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.68246666 09.01.2026 04:22:35.119 /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
First image: 2461049.68246666 09.01.2026 04:22:35.119 /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
Last image: 2461270.86617343 18.08.2026 08:47:07.384 /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 19
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.23
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 12 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 52195
Objects passed selection criteria: 52048
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 38256.2
Average stars matched: 35477 (92.7352 %)
Memory usage VmPeak: 271744 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 Tue Aug 18 04:03:12 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-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits
SExtractor catalog cache: saved Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits.cat to cache
SExtractor catalog cache: saved Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.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-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.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: 2461270.86523223
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-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits exists and is non-empty
wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits exists and is non-empty
wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits exists and is non-empty
wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits (1st reference image)
verification OK: wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
Image size: 941.6'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: 04:26:39.840 +13:59:58.72 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-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits (1st new image)
verification OK: wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits
Image size: 938.3'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: 04:26:21.567 +13:59:41.20 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 04:26:39.840 +13:59:58.72
Second-epoch image center 04:26:21.567 +13:59:41.20
Angular distance between the image centers 0.0740 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits (2nd new image)
verification OK: wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits
Image size: 938.2'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: 04:26:24.169 +14:00:26.31 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 04:26:39.840 +13:59:58.72
Second-epoch image center 04:26:24.169 +14:00:26.31
Angular distance between the image centers 0.0638 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 04:26:21.567 +13:59:41.20
Second-epoch second image center 04:26:24.169 +14:00:26.31
Angular distance between the image centers 0.01636 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-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits &> /tmp/tmp.zAl7GwNGPv
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits &> /tmp/tmp.Bp8WdU2QGn
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits &> /tmp/tmp.ZvJwfpmMCM
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits &> /tmp/tmp.nKKOrvuaMA
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.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-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits and wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.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-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits and wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits.wcscat
Found non-empty wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits and wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits.wcscat
The reference image (wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits) and catalog (wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits.wcscat) found
'wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits.wcscat' -> 'wcsmag.cat'
Read 9344 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 58.3894 to 74.9279 deg, Dec +8.6217 to +19.2873 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 58.3894 to 74.9279 deg, Dec 8.6217 to 19.2873 deg
Loaded 4391 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): 3406 out of 3669 total matches.
Matched with Tycho-2 3669 out of 9344 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.989100
a=0.000000 b=1.000000 c=22.989100
From vast_summary.log: estimated ref. image limiting mag.: -7.54
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.45
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.45
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 9344 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 58.3894 to 74.9279 deg, Dec +8.6217 to +19.2873 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 58.3894 to 74.9279 deg, Dec 8.6217 to 19.2873 deg
Loaded 4391 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): 3406 out of 3669 total matches.
Matched with Tycho-2 3669 out of 9344 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
Forced-photometry filter: calibrated wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits -> calib.txt_param_ref_wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits (aperture=6.0)
Read 8488 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 58.4321 to 74.9939 deg, Dec +8.6216 to +19.2870 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 58.4321 to 74.9939 deg, Dec 8.6216 to 19.2870 deg
Loaded 4407 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): 3395 out of 3650 total matches.
Matched with Tycho-2 3650 out of 8488 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits
Forced-photometry filter: calibrated wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits -> calib.txt_param_ref_wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits (aperture=5.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
2.0 pix Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits
2.5 pix fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits
2.4 pix fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits
Limiting magnitude estimates:
15.4 mag. Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
15.3 mag. Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits
14.4 mag. fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits
14.4 mag. fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 11.8 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.zAl7GwNGPv (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-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.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_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.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-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.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-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits' -> 'wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.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-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
WCS_IMAGE_NAME=wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
WCS-calibrated image found: wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
Checking if the catalog wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits.wcscat corresponding to the image wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits alredy exist and is non-empty...
Catalog wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits.wcscat corresponding to the image wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
WCS catalog name: wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.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=728, bad_region=1955, passed=9344
Got 9344 stars (including 6757 good ones) from the SExtractor catalog wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits.wcscat
util/solve_plate_with_UCAC5 got 9344 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 4887 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4874 matched stars entering correct_measured_positions(), 4874 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4874 matched stars entering correct_measured_positions(), 7722 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 4887 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4874 matched stars entering correct_measured_positions(), 7722 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 4874 matched stars entering correct_measured_positions(), 7722 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 4874 stars left (next iteration limit 5361)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits N_match=4874 sigma_overall_arcsec=0.304 sigma_q1_arcsec=0.377 sigma_q2_arcsec=0.311 sigma_q3_arcsec=0.269 sigma_q4_arcsec=0.270 n_q1=1649 n_q2=740 n_q3=1787 n_q4=698 worst_quadrant_to_overall_ratio=1.242
The image catalog is written to wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits -region wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.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.Bp8WdU2QGn (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-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.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_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.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-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.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-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits' -> 'wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.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-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits
WCS_IMAGE_NAME=wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits
WCS-calibrated image found: wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits
Checking if the catalog wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits.wcscat corresponding to the image wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits alredy exist and is non-empty...
Catalog wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits.wcscat corresponding to the image wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits
WCS catalog name: wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.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=679, bad_region=1868, passed=8488
Got 8488 stars (including 6040 good ones) from the SExtractor catalog wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits.wcscat
util/solve_plate_with_UCAC5 got 8488 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 4888 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4873 matched stars entering correct_measured_positions(), 4873 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4873 matched stars entering correct_measured_positions(), 6950 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4888 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4873 matched stars entering correct_measured_positions(), 6950 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4873 matched stars entering correct_measured_positions(), 6950 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4873 stars left (next iteration limit 5360)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits N_match=4873 sigma_overall_arcsec=0.345 sigma_q1_arcsec=0.483 sigma_q2_arcsec=0.322 sigma_q3_arcsec=0.303 sigma_q4_arcsec=0.257 n_q1=1626 n_q2=774 n_q3=1759 n_q4=714 worst_quadrant_to_overall_ratio=1.402
The image catalog is written to wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits -region wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.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.ZvJwfpmMCM (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_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.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_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits
WCS_IMAGE_NAME=wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits
WCS-calibrated image found: wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits
Checking if the catalog wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits.wcscat corresponding to the image wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits.wcscat corresponding to the image wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits
WCS catalog name: wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.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=357, bad_region=1552, passed=5731
Got 5731 stars (including 3920 good ones) from the SExtractor catalog wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits.wcscat
util/solve_plate_with_UCAC5 got 5731 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (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 0.010426 (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 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 3834 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3825 matched stars entering correct_measured_positions(), 3825 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3825 matched stars entering correct_measured_positions(), 4488 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
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 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 3834 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3826 matched stars entering correct_measured_positions(), 4488 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 3826 matched stars entering correct_measured_positions(), 4488 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 3826 stars left (next iteration limit 4207)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3826 robust_rms=7.089 arcsec worst_quadrant_rms=9.333 arcsec
SIP_REFIT: SIP order 3 trial: matched=3826 robust_rms=0.527 arcsec worst_quadrant_rms=0.585 arcsec
SIP_REFIT: SIP order 5 trial: matched=3826 robust_rms=0.460 arcsec worst_quadrant_rms=0.502 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3826 robust_rms_before=1.135 arcsec robust_rms_before_corrected=0.440 arcsec robust_rms_after=0.460 arcsec worst_quadrant_rms_before=0.461 worst_quadrant_rms_after=0.502
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.461 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits N_match=3826 sigma_overall_arcsec=0.443 sigma_q1_arcsec=0.422 sigma_q2_arcsec=0.457 sigma_q3_arcsec=0.451 sigma_q4_arcsec=0.478 n_q1=1161 n_q2=766 n_q3=1172 n_q4=727 worst_quadrant_to_overall_ratio=1.077
The image catalog is written to wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits -region wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.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.nKKOrvuaMA (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_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.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_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits
WCS_IMAGE_NAME=wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits
WCS-calibrated image found: wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits
Checking if the catalog wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits.wcscat corresponding to the image wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits.wcscat corresponding to the image wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits
WCS catalog name: wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.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=389, bad_region=1584, passed=5789
Got 5789 stars (including 3917 good ones) from the SExtractor catalog wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits.wcscat
util/solve_plate_with_UCAC5 got 5789 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.2'
Seting catalog search parameters based on the expected field of view 938.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013031 (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 0.010424 (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 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 3829 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3821 matched stars entering correct_measured_positions(), 3821 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3821 matched stars entering correct_measured_positions(), 4526 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
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 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 3829 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3822 matched stars entering correct_measured_positions(), 4526 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 3822 matched stars entering correct_measured_positions(), 4526 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 3822 stars left (next iteration limit 4203)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3822 robust_rms=7.023 arcsec worst_quadrant_rms=8.860 arcsec
SIP_REFIT: SIP order 3 trial: matched=3822 robust_rms=0.499 arcsec worst_quadrant_rms=0.544 arcsec
SIP_REFIT: SIP order 5 trial: matched=3822 robust_rms=0.442 arcsec worst_quadrant_rms=0.490 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3822 robust_rms_before=1.125 arcsec robust_rms_before_corrected=0.448 arcsec robust_rms_after=0.442 arcsec worst_quadrant_rms_before=0.482 worst_quadrant_rms_after=0.490
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.482 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits N_match=3822 sigma_overall_arcsec=0.456 sigma_q1_arcsec=0.421 sigma_q2_arcsec=0.505 sigma_q3_arcsec=0.442 sigma_q4_arcsec=0.496 n_q1=1153 n_q2=755 n_q3=1172 n_q4=742 worst_quadrant_to_overall_ratio=1.109
The image catalog is written to wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits -region wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.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-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits to local_wcs_cache/
'wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits' -> 'local_wcs_cache/wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits'
Saving the final (post-refit) wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits to local_wcs_cache/
'wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits' -> 'local_wcs_cache/wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits'
Saving the final (post-refit) wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits to local_wcs_cache/
'wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits' -> 'local_wcs_cache/wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits'
Saving the final (post-refit) wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits to local_wcs_cache/
'wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits' -> 'local_wcs_cache/wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits sigma_overall=0.304 worst_q_ratio=1.242
ref2=Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits sigma_overall=0.345 worst_q_ratio=1.402
new1=fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits sigma_overall=0.443 worst_q_ratio=1.077
new2=fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits sigma_overall=0.456 worst_q_ratio=1.109
reference average sigma_overall=0.3245 worst_q_ratio=1.322
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151_astrometric_residuals.png (4874 matched stars from wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147_astrometric_residuals.png (4873 matched stars from wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406_astrometric_residuals.png (3826 matched stars from wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.39 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407_astrometric_residuals.png (3822 matched stars from wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.40 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits'
Saving fully-calibrated image wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits'
Preparing the HTML report for the field Tau-06-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20116_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407
The candidate 20116_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407 did not pass the final checks
**** FOUND 04:27:51.56 +10:00:50.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02564_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407
The candidate 02564_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407 did not pass the final checks
**** FOUND 04:25:27.21 +16:33:21.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06530_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407
The candidate 06530_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407 did not pass the final checks
**** FOUND 04:43:23.97 +11:35:06.0 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Tau-06-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-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits
SExtractor catalog cache: saved Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits.cat to cache
SExtractor catalog cache: saved Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.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-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
Creating symlink local_wcs_cache/wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.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-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits exists and is non-empty
wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits exists and is non-empty
wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits exists and is non-empty
wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits (1st reference image)
verification OK: wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
Image size: 941.6'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: 04:26:39.840 +13:59:58.72 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-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits (1st new image)
verification OK: wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits
Image size: 938.3'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: 04:26:21.567 +13:59:41.20 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 04:26:39.840 +13:59:58.72
Second-epoch image center 04:26:21.567 +13:59:41.20
Angular distance between the image centers 0.0740 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits (2nd new image)
verification OK: wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits
Image size: 938.2'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: 04:26:24.169 +14:00:26.31 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 04:26:39.840 +13:59:58.72
Second-epoch image center 04:26:24.169 +14:00:26.31
Angular distance between the image centers 0.0638 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 04:26:21.567 +13:59:41.20
Second-epoch second image center 04:26:24.169 +14:00:26.31
Angular distance between the image centers 0.01636 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-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits &> /tmp/tmp.xVNByM2pRF
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits &> /tmp/tmp.in7MGCs2Da
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits &> /tmp/tmp.fLYpTzVfc0
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits &> /tmp/tmp.uhBOEXKZVq
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.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-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits and wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.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-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits and wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits.wcscat
Found non-empty wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits and wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits.wcscat
The reference image (wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits) and catalog (wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits.wcscat) found
'wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits.wcscat' -> 'wcsmag.cat'
Read 62263 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 58.3895 to 74.9801 deg, Dec +8.6217 to +19.2873 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 58.3895 to 74.9801 deg, Dec 8.6217 to 19.2873 deg
Loaded 4417 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): 3083 out of 3672 total matches.
Matched with Tycho-2 3672 out of 62263 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.852800
a=0.000000 b=1.000000 c=22.852800
From vast_summary.log: estimated ref. image limiting mag.: -7.23
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.62
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.62
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 62263 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 58.3895 to 74.9801 deg, Dec +8.6217 to +19.2873 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 58.3895 to 74.9801 deg, Dec 8.6217 to 19.2873 deg
Loaded 4417 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): 3083 out of 3672 total matches.
Matched with Tycho-2 3672 out of 62263 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
Forced-photometry filter: calibrated wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits -> calib.txt_param_ref_wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits (aperture=4.5)
Read 58309 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 58.4014 to 74.9981 deg, Dec +8.6064 to +19.2869 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 58.4014 to 74.9981 deg, Dec 8.6064 to 19.2869 deg
Loaded 4433 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): 3131 out of 3673 total matches.
Matched with Tycho-2 3673 out of 58309 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits
Forced-photometry filter: calibrated wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits -> calib.txt_param_ref_wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits (aperture=4.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 17 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
1.8 pix Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits
2.3 pix fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits
2.3 pix fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits
Limiting magnitude estimates:
15.6 mag. Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
15.5 mag. Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits
14.7 mag. fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits
14.7 mag. fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 14.3 (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.xVNByM2pRF (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-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.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_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.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-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.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-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits' -> 'wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.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-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
WCS_IMAGE_NAME=wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
WCS-calibrated image found: wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
Checking if the catalog wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits.wcscat corresponding to the image wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits alredy exist and is non-empty...
Catalog wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits.wcscat corresponding to the image wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
WCS catalog name: wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.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=12, blended=3506, bad_region=10392, passed=62251
Got 62251 stars (including 48725 good ones) from the SExtractor catalog wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits.wcscat
util/solve_plate_with_UCAC5 got 62251 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 4890 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4881 matched stars entering correct_measured_positions(), 4881 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4881 matched stars entering correct_measured_positions(), 53920 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 4890 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4881 matched stars entering correct_measured_positions(), 53920 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 4881 matched stars entering correct_measured_positions(), 53920 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4881 stars left (next iteration limit 5369)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.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-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits N_match=4881 sigma_overall_arcsec=0.302 sigma_q1_arcsec=0.367 sigma_q2_arcsec=0.319 sigma_q3_arcsec=0.270 sigma_q4_arcsec=0.258 n_q1=1624 n_q2=735 n_q3=1801 n_q4=721 worst_quadrant_to_overall_ratio=1.213
The image catalog is written to wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits -region wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.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.in7MGCs2Da (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-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.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_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.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-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.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-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits' -> 'wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.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-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits
WCS_IMAGE_NAME=wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits
WCS-calibrated image found: wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits
Checking if the catalog wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits.wcscat corresponding to the image wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits alredy exist and is non-empty...
Catalog wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits.wcscat corresponding to the image wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits
WCS catalog name: wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.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=6, blended=3080, bad_region=9253, passed=58303
Got 58303 stars (including 46293 good ones) from the SExtractor catalog wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits.wcscat
util/solve_plate_with_UCAC5 got 58303 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 4891 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4880 matched stars entering correct_measured_positions(), 4880 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4880 matched stars entering correct_measured_positions(), 50853 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4891 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4880 matched stars entering correct_measured_positions(), 50853 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4880 matched stars entering correct_measured_positions(), 50854 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4880 stars left (next iteration limit 5368)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.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-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits N_match=4880 sigma_overall_arcsec=0.333 sigma_q1_arcsec=0.462 sigma_q2_arcsec=0.310 sigma_q3_arcsec=0.301 sigma_q4_arcsec=0.251 n_q1=1612 n_q2=760 n_q3=1786 n_q4=722 worst_quadrant_to_overall_ratio=1.387
The image catalog is written to wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits -region wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.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.fLYpTzVfc0 (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_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.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_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits
WCS_IMAGE_NAME=wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits
WCS-calibrated image found: wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits
Checking if the catalog wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits.wcscat corresponding to the image wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits.wcscat corresponding to the image wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits
WCS catalog name: wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.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=6, blended=1422, bad_region=6538, passed=33002
Got 33002 stars (including 25460 good ones) from the SExtractor catalog wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits.wcscat
util/solve_plate_with_UCAC5 got 33002 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (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 0.010426 (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 492 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: 4885 matched stars entering correct_measured_positions(), 4885 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4885 matched stars entering correct_measured_positions(), 28053 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
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 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4896 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4886 matched stars entering correct_measured_positions(), 28053 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 4886 matched stars entering correct_measured_positions(), 28053 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 4886 stars left (next iteration limit 5373)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.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=4886 robust_rms=6.898 arcsec worst_quadrant_rms=10.725 arcsec
SIP_REFIT: SIP order 3 trial: matched=4886 robust_rms=0.530 arcsec worst_quadrant_rms=0.586 arcsec
SIP_REFIT: SIP order 5 trial: matched=4886 robust_rms=0.460 arcsec worst_quadrant_rms=0.507 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4886 robust_rms_before=1.137 arcsec robust_rms_before_corrected=0.431 arcsec robust_rms_after=0.460 arcsec worst_quadrant_rms_before=0.450 worst_quadrant_rms_after=0.507
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.450 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits N_match=4886 sigma_overall_arcsec=0.437 sigma_q1_arcsec=0.413 sigma_q2_arcsec=0.446 sigma_q3_arcsec=0.440 sigma_q4_arcsec=0.481 n_q1=1482 n_q2=923 n_q3=1535 n_q4=946 worst_quadrant_to_overall_ratio=1.102
The image catalog is written to wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits -region wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.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.uhBOEXKZVq (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_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.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_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits
WCS_IMAGE_NAME=wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits
WCS-calibrated image found: wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits
Checking if the catalog wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits.wcscat corresponding to the image wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits.wcscat corresponding to the image wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits
WCS catalog name: wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=1436, bad_region=6650, passed=33384
Got 33384 stars (including 25716 good ones) from the SExtractor catalog wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits.wcscat
util/solve_plate_with_UCAC5 got 33384 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.2'
Seting catalog search parameters based on the expected field of view 938.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013031 (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 0.010424 (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 492 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
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: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4883 matched stars entering correct_measured_positions(), 28354 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
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 492 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(), 28354 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 4883 matched stars entering correct_measured_positions(), 28354 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
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-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.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=6.788 arcsec worst_quadrant_rms=9.945 arcsec
SIP_REFIT: SIP order 3 trial: matched=4883 robust_rms=0.506 arcsec worst_quadrant_rms=0.532 arcsec
SIP_REFIT: SIP order 5 trial: matched=4883 robust_rms=0.448 arcsec worst_quadrant_rms=0.488 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4883 robust_rms_before=1.125 arcsec robust_rms_before_corrected=0.436 arcsec robust_rms_after=0.448 arcsec worst_quadrant_rms_before=0.475 worst_quadrant_rms_after=0.488
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-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits N_match=4883 sigma_overall_arcsec=0.438 sigma_q1_arcsec=0.426 sigma_q2_arcsec=0.474 sigma_q3_arcsec=0.444 sigma_q4_arcsec=0.474 n_q1=1488 n_q2=921 n_q3=1531 n_q4=943 worst_quadrant_to_overall_ratio=1.082
The image catalog is written to wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits -region wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.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-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.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_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-45-46_20.00sec_-0.00C_LIGHT_0406.fits
Saving fully-calibrated image wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.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_2026-08-18_CI_Tau-06-Q2b1x1_035254_TTUQ2b1x1_1930021_iEpbkA0n/wcs_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407.fits
Preparing the HTML report for the field Tau-06-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits at 04:39:53.18 +17:06:06.4: 16.24 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits at 04:19:16.11 +16:12:56.1: 14.99 +/- 0.11 detection
Forced photometry on wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits at 04:38:25.96 +16:18:51.3: 16.23 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-06-Q2b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits at 04:15:55.49 +13:09:50.6: 14.48 +/- 0.09 detection
Forced photometry on wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits at 04:39:53.18 +17:06:06.4: 16.15 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits at 04:15:55.49 +13:09:50.6: 14.24 +/- 0.08 detection
Forced photometry on wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits at 04:19:16.11 +16:12:56.1: 15.29 +/- 0.16 detection
Forced photometry on wcs_Tau-06-Q2b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits at 04:38:25.96 +16:18:51.3: 16.17 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.09 +/- 0.09
Forced photometry reference-image weighted average: 14.34 +/- 0.06
Forced photometry filter REJECTED candidate at 04:19:16.11 +16:12:56.1: ref_mag=15.09 +/- 0.09 new_mean_mag=14.7381 delta=0.35 (need > 0.90)
Forced photometry filter REJECTED candidate at 04:15:55.49 +13:09:50.6: ref_mag=14.34 +/- 0.06 new_mean_mag=14.2801 delta=0.06 (need > 0.90)
Adding exclusion_list_local.txt__out79472.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out80367.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
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: 2s
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Considering the candidate 75336_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407
The candidate 75336_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407 did not pass the final checks
**** FOUND 04:19:54.85 +10:10:24.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 76420_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407
The candidate 76420_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407 did not pass the final checks
**** FOUND 04:26:24.85 +15:35:08.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78154_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407
The candidate 78154_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407 did not pass the final checks
**** FOUND 04:21:59.67 +14:06:14.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 78355_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407
The candidate 78355_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407 did not pass the final checks
**** FOUND 04:38:35.54 +17:25:28.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78724_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407
The candidate 78724_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407 did not pass the final checks
**** FOUND 04:30:08.16 +15:39:58.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 78802_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407
The candidate 78802_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407 did not pass the final checks
**** FOUND 04:30:13.69 +15:39:25.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 78923_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407
The candidate 78923_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407 did not pass the final checks
**** FOUND 04:35:39.11 +16:08:29.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79069_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407
The candidate 79069_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407 did not pass the final checks
**** FOUND 04:33:58.27 +10:13:55.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79409_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407
The candidate 79409_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407 did not pass the final checks
**** FOUND 04:33:52.77 +13:15:17.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79472_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407
Preparing report for the candidate 79472_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407
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Considering the candidate 79480_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407
The candidate 79480_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407 did not pass the final checks
**** FOUND 04:21:31.35 +14:25:59.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79693_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407
The candidate 79693_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407 did not pass the final checks
**** FOUND 04:20:48.61 +13:50:46.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 80257_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407
The candidate 80257_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407 did not pass the final checks
**** FOUND 04:34:19.06 +12:36:41.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 80367_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407
Preparing report for the candidate 80367_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407
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Considering the candidate 82241_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407
The candidate 82241_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407 did not pass the final checks
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Considering the candidate 82322_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407
The candidate 82322_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407 did not pass the final checks
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Considering the candidate 56370_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407
The candidate 56370_fd_Tau-06-Q2b1x1_2026-08-18_03-47-07_20.00sec_-0.00C_LIGHT_0407 did not pass the final checks