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-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y
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 18.3673 2461270.8673 13.66 04:39:53.35 +17:06:05.9
181.09470 -19.13496 galactic Tau Second-epoch detections are separated by 0.6" and 9.4 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 -0 0 13.6 -0 0
Forced photometry on wcs_Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits at 04:39:53.35 +17:06:05.9: 16.24 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-06-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits at 04:39:53.35 +17:06:05.9: 16.13 +/- 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 18.3672* 04 39 53.35 +17 06 05.9 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,2461270.8673,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260818.3673 13.66CV 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 18.3673 2461270.8673 13.94 04:38:26.11 +16:18:50.4
181.53007 -19.89205 galactic Tau Second-epoch detections are separated by 0.9" and 9.4 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 -1 2 14.3 0 0
Forced photometry on wcs_Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits at 04:38:26.11 +16:18:50.4: 16.23 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-06-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits at 04:38:26.11 +16:18:50.4: 16.16 +/- 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 18.3672* 04 38 26.11 +16 18 50.4 13.9 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,2461270.8673,13.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260818.3673 13.94CV 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-Q1b1x1_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-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
Last image: 2461270.86772949 18.08.2026 08:49:21.828 /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
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: 4 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): 8468
Objects passed selection criteria: 8454
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 7544.5
Average stars matched: 7439.75 (98.6116 %)
Memory usage VmPeak: 234636 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 03:56:09 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-Q1b1x1_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-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
Last image: 2461270.86772949 18.08.2026 08:49:21.828 /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 32
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.24
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 16 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 55513
Objects passed selection criteria: 55396
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 45664.2
Average stars matched: 44403.8 (97.2396 %)
Memory usage VmPeak: 277252 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 03:57:00 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/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q1b1x1_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-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits
SExtractor catalog cache: saved Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits.cat to cache
SExtractor catalog cache: saved Tau-06-Q1b1x1_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-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q1b1x1_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-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.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: 2461270.86677332
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-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits exists and is non-empty
wcs_Tau-06-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits exists and is non-empty
wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits exists and is non-empty
wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits (1st reference image)
verification OK: wcs_Tau-06-Q1b1x1_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-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits (1st new image)
verification OK: wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits
Image size: 942.2'x626.8' 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: 04:26:35.697 +13:58:47.15 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 04:26:35.697 +13:58:47.15
Angular distance between the image centers 0.0260 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits (2nd new image)
verification OK: wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits
Image size: 942.2'x626.8' 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: 04:26:38.602 +13:58:09.13 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 04:26:38.602 +13:58:09.13
Angular distance between the image centers 0.0308 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 04:26:35.697 +13:58:47.15
Second-epoch second image center 04:26:38.602 +13:58:09.13
Angular distance between the image centers 0.01580 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-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits &> /tmp/tmp.bMCfXdFvkH
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q1b1x1_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-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits &> /tmp/tmp.2Tfsqn5ElJ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q1b1x1_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-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits &> /tmp/tmp.2MuRU2goSz
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits &> /tmp/tmp.1IoORLEUml
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-06-Q1b1x1_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-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits and wcs_Tau-06-Q1b1x1_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-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits and wcs_Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits.wcscat
Found non-empty wcs_Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits and wcs_Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits.wcscat
The reference image (wcs_Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits) and catalog (wcs_Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits.wcscat) found
'wcs_Tau-06-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
Forced-photometry filter: calibrated wcs_Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits -> calib.txt_param_ref_wcs_Tau-06-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits
Forced-photometry filter: calibrated wcs_Tau-06-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits -> calib.txt_param_ref_wcs_Tau-06-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits (aperture=5.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
2.0 pix Tau-06-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits
3.0 pix fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits
3.0 pix fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits
Limiting magnitude estimates:
15.4 mag. Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
15.3 mag. Tau-06-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits
14.2 mag. fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits
14.2 mag. fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 11.9 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.bMCfXdFvkH (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-18_CI_Tau-06-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits' -> 'wcs_Tau-06-Q1b1x1_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-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
WCS_IMAGE_NAME=wcs_Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
WCS-calibrated image found: wcs_Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
Checking if the catalog wcs_Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits.wcscat corresponding to the image wcs_Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits alredy exist and is non-empty...
Catalog wcs_Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits.wcscat corresponding to the image wcs_Tau-06-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
WCS catalog name: wcs_Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=728, bad_region=0, passed=9344
Got 9344 stars (including 8597 good ones) from the SExtractor catalog wcs_Tau-06-Q1b1x1_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 4892 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(), 9344 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
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 4892 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(), 9344 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 4881 matched stars entering correct_measured_positions(), 9344 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 4881 stars left (next iteration limit 5369)
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-Q1b1x1_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-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits N_match=4881 sigma_overall_arcsec=0.294 sigma_q1_arcsec=0.372 sigma_q2_arcsec=0.304 sigma_q3_arcsec=0.264 sigma_q4_arcsec=0.258 n_q1=1309 n_q2=1102 n_q3=1429 n_q4=1041 worst_quadrant_to_overall_ratio=1.263
The image catalog is written to wcs_Tau-06-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits -region wcs_Tau-06-Q1b1x1_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-Q1b1x1_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.2Tfsqn5ElJ (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-18_CI_Tau-06-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits' -> 'wcs_Tau-06-Q1b1x1_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-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits
WCS_IMAGE_NAME=wcs_Tau-06-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits
WCS-calibrated image found: wcs_Tau-06-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits
Checking if the catalog wcs_Tau-06-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits.wcscat corresponding to the image wcs_Tau-06-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits alredy exist and is non-empty...
Catalog wcs_Tau-06-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits.wcscat corresponding to the image wcs_Tau-06-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits
WCS catalog name: wcs_Tau-06-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=679, bad_region=1, passed=8488
Got 8488 stars (including 7793 good ones) from the SExtractor catalog wcs_Tau-06-Q1b1x1_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 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: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4883 matched stars entering correct_measured_positions(), 8488 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 4893 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4882 matched stars entering correct_measured_positions(), 8488 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4882 matched stars entering correct_measured_positions(), 8488 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4882 stars left (next iteration limit 5371)
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-Q1b1x1_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-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits N_match=4882 sigma_overall_arcsec=0.322 sigma_q1_arcsec=0.474 sigma_q2_arcsec=0.299 sigma_q3_arcsec=0.302 sigma_q4_arcsec=0.242 n_q1=1282 n_q2=1141 n_q3=1405 n_q4=1054 worst_quadrant_to_overall_ratio=1.472
The image catalog is written to wcs_Tau-06-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits -region wcs_Tau-06-Q1b1x1_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-Q1b1x1_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.2MuRU2goSz (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-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.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-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits
WCS_IMAGE_NAME=wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits
WCS-calibrated image found: wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits
Checking if the catalog wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits.wcscat corresponding to the image wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits.wcscat corresponding to the image wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.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-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits
WCS catalog name: wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=319, bad_region=0, passed=6277
Got 6277 stars (including 5954 good ones) from the SExtractor catalog wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits.wcscat
util/solve_plate_with_UCAC5 got 6277 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.2'
Seting catalog search parameters based on the expected field of view 942.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013086 (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 0.010469 (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 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 4882 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4867 matched stars entering correct_measured_positions(), 4867 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4867 matched stars entering correct_measured_positions(), 6277 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
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 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 4881 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4867 matched stars entering correct_measured_positions(), 6277 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 4867 matched stars entering correct_measured_positions(), 6277 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 4867 stars left (next iteration limit 5353)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4867 robust_rms=12.123 arcsec worst_quadrant_rms=13.324 arcsec
SIP_REFIT: SIP order 3 trial: matched=4867 robust_rms=0.485 arcsec worst_quadrant_rms=0.629 arcsec
SIP_REFIT: SIP order 5 trial: matched=4867 robust_rms=0.383 arcsec worst_quadrant_rms=0.475 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4867 robust_rms_before=1.144 arcsec robust_rms_before_corrected=0.373 arcsec robust_rms_after=0.383 arcsec worst_quadrant_rms_before=0.482 worst_quadrant_rms_after=0.475
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-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits N_match=4867 sigma_overall_arcsec=0.367 sigma_q1_arcsec=0.337 sigma_q2_arcsec=0.468 sigma_q3_arcsec=0.283 sigma_q4_arcsec=0.405 n_q1=1091 n_q2=1311 n_q3=1191 n_q4=1274 worst_quadrant_to_overall_ratio=1.274
The image catalog is written to wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits -region wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.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.1IoORLEUml (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-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.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-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits
WCS_IMAGE_NAME=wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits
WCS-calibrated image found: wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits
Checking if the catalog wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits.wcscat corresponding to the image wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits.wcscat corresponding to the image wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.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-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits
WCS catalog name: wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=1, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=343, bad_region=0, passed=6313
Got 6313 stars (including 5965 good ones) from the SExtractor catalog wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits.wcscat
util/solve_plate_with_UCAC5 got 6313 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.2'
Seting catalog search parameters based on the expected field of view 942.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013086 (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 0.010469 (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 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 4881 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4867 matched stars entering correct_measured_positions(), 4867 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4867 matched stars entering correct_measured_positions(), 6313 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
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 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 4881 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4867 matched stars entering correct_measured_positions(), 6313 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 4867 matched stars entering correct_measured_positions(), 6313 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 4867 stars left (next iteration limit 5353)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4867 robust_rms=12.253 arcsec worst_quadrant_rms=13.414 arcsec
SIP_REFIT: SIP order 3 trial: matched=4867 robust_rms=0.479 arcsec worst_quadrant_rms=0.628 arcsec
SIP_REFIT: SIP order 5 trial: matched=4867 robust_rms=0.397 arcsec worst_quadrant_rms=0.511 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4867 robust_rms_before=1.152 arcsec robust_rms_before_corrected=0.373 arcsec robust_rms_after=0.397 arcsec worst_quadrant_rms_before=0.492 worst_quadrant_rms_after=0.511
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.492 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits N_match=4867 sigma_overall_arcsec=0.372 sigma_q1_arcsec=0.349 sigma_q2_arcsec=0.478 sigma_q3_arcsec=0.285 sigma_q4_arcsec=0.413 n_q1=1094 n_q2=1299 n_q3=1202 n_q4=1272 worst_quadrant_to_overall_ratio=1.286
The image catalog is written to wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits -region wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.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-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits to local_wcs_cache/
'wcs_Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits' -> 'local_wcs_cache/wcs_Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits'
Saving the final (post-refit) wcs_Tau-06-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits to local_wcs_cache/
'wcs_Tau-06-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits' -> 'local_wcs_cache/wcs_Tau-06-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits'
Saving the final (post-refit) wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits to local_wcs_cache/
'wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits' -> 'local_wcs_cache/wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits'
Saving the final (post-refit) wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits to local_wcs_cache/
'wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits' -> 'local_wcs_cache/wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits sigma_overall=0.294 worst_q_ratio=1.263
ref2=Tau-06-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits sigma_overall=0.322 worst_q_ratio=1.472
new1=fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits sigma_overall=0.367 worst_q_ratio=1.274
new2=fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits sigma_overall=0.372 worst_q_ratio=1.286
reference average sigma_overall=0.308 worst_q_ratio=1.3675
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151_astrometric_residuals.png (4881 matched stars from wcs_Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.26 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Tau-06-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147_astrometric_residuals.png (4882 matched stars from wcs_Tau-06-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374_astrometric_residuals.png (4867 matched stars from wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.33 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375_astrometric_residuals.png (4867 matched stars from wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.33 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits'
Saving fully-calibrated image wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits'
Preparing the HTML report for the field Tau-06-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20337_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375
The candidate 20337_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375 did not pass the final checks
**** FOUND 04:54:18.50 +11:10:44.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02564_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375
The candidate 02564_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375 did not pass the final checks
**** FOUND 04:25:27.21 +16:33:23.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06530_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375
The candidate 06530_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375 did not pass the final checks
**** FOUND 04:43:23.98 +11:35:05.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01595_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375
The candidate 01595_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375 did not pass the final checks
**** FOUND 04:52:02.19 +17:32:15.4 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-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q1b1x1_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-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits
SExtractor catalog cache: saved Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits.cat to cache
SExtractor catalog cache: saved Tau-06-Q1b1x1_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-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q1b1x1_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-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
Creating symlink local_wcs_cache/wcs_Tau-06-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.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-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits exists and is non-empty
wcs_Tau-06-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits exists and is non-empty
wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits exists and is non-empty
wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits (1st reference image)
verification OK: wcs_Tau-06-Q1b1x1_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-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits (1st new image)
verification OK: wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits
Image size: 942.2'x626.8' 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: 04:26:35.697 +13:58:47.15 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 04:26:35.697 +13:58:47.15
Angular distance between the image centers 0.0260 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits (2nd new image)
verification OK: wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits
Image size: 942.2'x626.8' 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: 04:26:38.602 +13:58:09.13 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 04:26:38.602 +13:58:09.13
Angular distance between the image centers 0.0308 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 04:26:35.697 +13:58:47.15
Second-epoch second image center 04:26:38.602 +13:58:09.13
Angular distance between the image centers 0.01580 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-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits &> /tmp/tmp.QQFBvdhbpW
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q1b1x1_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-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits &> /tmp/tmp.ig12hPZPWp
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q1b1x1_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-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits &> /tmp/tmp.Qz73KTM4DK
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits &> /tmp/tmp.2fEHFnFaNI
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-06-Q1b1x1_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-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits and wcs_Tau-06-Q1b1x1_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-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits and wcs_Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits.wcscat
Found non-empty wcs_Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits and wcs_Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits.wcscat
The reference image (wcs_Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits) and catalog (wcs_Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits.wcscat) found
'wcs_Tau-06-Q1b1x1_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.: -7.24
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.61
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.61
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
Forced-photometry filter: calibrated wcs_Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits -> calib.txt_param_ref_wcs_Tau-06-Q1b1x1_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-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits
Forced-photometry filter: calibrated wcs_Tau-06-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits -> calib.txt_param_ref_wcs_Tau-06-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits (aperture=4.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 26 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
1.8 pix Tau-06-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits
2.9 pix fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits
2.9 pix fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits
Limiting magnitude estimates:
15.6 mag. Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
15.5 mag. Tau-06-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits
14.6 mag. fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits
14.6 mag. fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 14.1 (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.QQFBvdhbpW (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-18_CI_Tau-06-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits' -> 'wcs_Tau-06-Q1b1x1_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-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
WCS_IMAGE_NAME=wcs_Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
WCS-calibrated image found: wcs_Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
Checking if the catalog wcs_Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits.wcscat corresponding to the image wcs_Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits alredy exist and is non-empty...
Catalog wcs_Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits.wcscat corresponding to the image wcs_Tau-06-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits
WCS catalog name: wcs_Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=3506, bad_region=5, passed=62251
Got 62251 stars (including 58597 good ones) from the SExtractor catalog wcs_Tau-06-Q1b1x1_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 4892 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: 0.25"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4885 matched stars entering correct_measured_positions(), 62251 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 4892 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4885 matched stars entering correct_measured_positions(), 62251 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 4885 matched stars entering correct_measured_positions(), 62251 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 4885 stars left (next iteration limit 5373)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Tau-06-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits N_match=4885 sigma_overall_arcsec=0.296 sigma_q1_arcsec=0.373 sigma_q2_arcsec=0.312 sigma_q3_arcsec=0.260 sigma_q4_arcsec=0.258 n_q1=1302 n_q2=1091 n_q3=1432 n_q4=1060 worst_quadrant_to_overall_ratio=1.258
The image catalog is written to wcs_Tau-06-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits -region wcs_Tau-06-Q1b1x1_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-Q1b1x1_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.ig12hPZPWp (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-18_CI_Tau-06-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-06-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits' -> 'wcs_Tau-06-Q1b1x1_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-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits
WCS_IMAGE_NAME=wcs_Tau-06-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits
WCS-calibrated image found: wcs_Tau-06-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits
Checking if the catalog wcs_Tau-06-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits.wcscat corresponding to the image wcs_Tau-06-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits alredy exist and is non-empty...
Catalog wcs_Tau-06-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits.wcscat corresponding to the image wcs_Tau-06-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits
WCS catalog name: wcs_Tau-06-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=3080, bad_region=5, passed=58299
Got 58299 stars (including 55093 good ones) from the SExtractor catalog wcs_Tau-06-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits.wcscat
util/solve_plate_with_UCAC5 got 58299 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 4893 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4884 matched stars entering correct_measured_positions(), 4884 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4884 matched stars entering correct_measured_positions(), 58299 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4893 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4884 matched stars entering correct_measured_positions(), 58299 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4884 matched stars entering correct_measured_positions(), 58299 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4884 stars left (next iteration limit 5372)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Tau-06-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits N_match=4884 sigma_overall_arcsec=0.316 sigma_q1_arcsec=0.470 sigma_q2_arcsec=0.304 sigma_q3_arcsec=0.299 sigma_q4_arcsec=0.235 n_q1=1266 n_q2=1129 n_q3=1416 n_q4=1073 worst_quadrant_to_overall_ratio=1.486
The image catalog is written to wcs_Tau-06-Q1b1x1_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-Q1b1x1_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-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits -region wcs_Tau-06-Q1b1x1_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-Q1b1x1_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.Qz73KTM4DK (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-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.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-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits
WCS_IMAGE_NAME=wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits
WCS-calibrated image found: wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits
Checking if the catalog wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits.wcscat corresponding to the image wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits.wcscat corresponding to the image wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.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-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits
WCS catalog name: wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=1171, bad_region=37, passed=32017
Got 32017 stars (including 30753 good ones) from the SExtractor catalog wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits.wcscat
util/solve_plate_with_UCAC5 got 32017 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.2'
Seting catalog search parameters based on the expected field of view 942.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013086 (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 0.010469 (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 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 4885 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4870 matched stars entering correct_measured_positions(), 4870 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4870 matched stars entering correct_measured_positions(), 32017 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 4884 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4869 matched stars entering correct_measured_positions(), 32017 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 4869 matched stars entering correct_measured_positions(), 32017 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 4869 stars left (next iteration limit 5357)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.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=4869 robust_rms=12.450 arcsec worst_quadrant_rms=13.213 arcsec
SIP_REFIT: SIP order 3 trial: matched=4869 robust_rms=0.488 arcsec worst_quadrant_rms=0.615 arcsec
SIP_REFIT: SIP order 5 trial: matched=4869 robust_rms=0.384 arcsec worst_quadrant_rms=0.471 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4869 robust_rms_before=1.137 arcsec robust_rms_before_corrected=0.374 arcsec robust_rms_after=0.384 arcsec worst_quadrant_rms_before=0.468 worst_quadrant_rms_after=0.471
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.468 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits N_match=4869 sigma_overall_arcsec=0.374 sigma_q1_arcsec=0.346 sigma_q2_arcsec=0.466 sigma_q3_arcsec=0.290 sigma_q4_arcsec=0.404 n_q1=1109 n_q2=1283 n_q3=1217 n_q4=1260 worst_quadrant_to_overall_ratio=1.247
The image catalog is written to wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits -region wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.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.2fEHFnFaNI (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-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.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-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits
WCS_IMAGE_NAME=wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits
WCS-calibrated image found: wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits
Checking if the catalog wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits.wcscat corresponding to the image wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits.wcscat corresponding to the image wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.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-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits
WCS catalog name: wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=1268, bad_region=39, passed=31616
Got 31616 stars (including 30253 good ones) from the SExtractor catalog wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits.wcscat
util/solve_plate_with_UCAC5 got 31616 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.2'
Seting catalog search parameters based on the expected field of view 942.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013086 (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 0.010469 (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 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 4882 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4868 matched stars entering correct_measured_positions(), 4868 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4868 matched stars entering correct_measured_positions(), 31616 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
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 491 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 4882 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4868 matched stars entering correct_measured_positions(), 31616 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4868 matched stars entering correct_measured_positions(), 31616 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 4868 stars left (next iteration limit 5354)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.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=4868 robust_rms=12.602 arcsec worst_quadrant_rms=13.343 arcsec
SIP_REFIT: SIP order 3 trial: matched=4868 robust_rms=0.480 arcsec worst_quadrant_rms=0.616 arcsec
SIP_REFIT: SIP order 5 trial: matched=4868 robust_rms=0.396 arcsec worst_quadrant_rms=0.510 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4868 robust_rms_before=1.150 arcsec robust_rms_before_corrected=0.380 arcsec robust_rms_after=0.396 arcsec worst_quadrant_rms_before=0.483 worst_quadrant_rms_after=0.510
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.483 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits N_match=4868 sigma_overall_arcsec=0.373 sigma_q1_arcsec=0.347 sigma_q2_arcsec=0.484 sigma_q3_arcsec=0.281 sigma_q4_arcsec=0.418 n_q1=1104 n_q2=1277 n_q3=1227 n_q4=1260 worst_quadrant_to_overall_ratio=1.297
The image catalog is written to wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Tau-06-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits -region wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.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-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.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-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-47-59_20.00sec_-0.00C_LIGHTs_0374.fits
Saving fully-calibrated image wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.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-Q1b1x1_035052_TTUQ1b1x1_1254157_Ow2ZkR0y/wcs_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375.fits
Preparing the HTML report for the field Tau-06-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits at 04:39:11.16 +17:52:56.9: 13.68 +/- 0.04 detection
Forced photometry on wcs_Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits at 04:12:12.35 +12:22:20.0: 14.08 +/- 0.05 detection
Forced photometry on wcs_Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits at 04:38:35.50 +17:25:29.3: 13.60 +/- 0.04 detection
Forced photometry on wcs_Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits at 04:39:53.35 +17:06:05.9: 16.24 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits at 04:38:26.11 +16:18:50.4: 16.23 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits at 04:34:19.06 +12:36:40.3: 13.86 +/- 0.05 detection
Forced photometry on wcs_Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits at 04:21:31.37 +14:25:58.4: 13.93 +/- 0.05 detection
Forced photometry on wcs_Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits at 04:35:39.12 +16:08:31.9: 13.67 +/- 0.04 detection
Forced photometry on wcs_Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits at 04:25:38.54 +17:55:22.4: 13.89 +/- 0.06 detection
Forced photometry on wcs_Tau-06-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits at 04:12:12.35 +12:22:20.0: 13.97 +/- 0.05 detection
Forced photometry on wcs_Tau-06-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits at 04:39:11.16 +17:52:56.9: 13.76 +/- 0.04 detection
Forced photometry reference-image weighted average: 14.03 +/- 0.03
Forced photometry reference-image weighted average: 13.71 +/- 0.03
Forced photometry filter REJECTED candidate at 04:12:12.35 +12:22:20.0: ref_mag=14.03 +/- 0.03 new_mean_mag=13.9225 delta=0.11 (need > 0.90)
Forced photometry filter REJECTED candidate at 04:39:11.16 +17:52:56.9: ref_mag=13.71 +/- 0.03 new_mean_mag=13.5144 delta=0.20 (need > 0.90)
Forced photometry on wcs_Tau-06-Q1b1x1_2026-01-08_22-22-35_20.00sec_-14.90C_LIGHT_0151.fits at 04:37:05.84 +15:55:35.0: 14.07 +/- 0.06 detection
Forced photometry on wcs_Tau-06-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits at 04:38:35.50 +17:25:29.3: 13.55 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.57 +/- 0.03
Forced photometry filter REJECTED candidate at 04:38:35.50 +17:25:29.3: ref_mag=13.57 +/- 0.03 new_mean_mag=13.4193 delta=0.15 (need > 0.90)
Forced photometry on wcs_Tau-06-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits at 04:38:26.11 +16:18:50.4: 16.16 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-06-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits at 04:34:19.06 +12:36:40.3: 13.84 +/- 0.05 detection
Forced photometry on wcs_Tau-06-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits at 04:21:31.37 +14:25:58.4: 13.90 +/- 0.05 detection
Forced photometry on wcs_Tau-06-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits at 04:35:39.12 +16:08:31.9: 13.66 +/- 0.04 detection
Forced photometry on wcs_Tau-06-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits at 04:39:53.35 +17:06:05.9: 16.13 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.85 +/- 0.04
Forced photometry reference-image weighted average: 13.91 +/- 0.03
Forced photometry on wcs_Tau-06-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits at 04:25:38.54 +17:55:22.4: 13.98 +/- 0.07 detection
Forced photometry filter REJECTED candidate at 04:34:19.06 +12:36:40.3: ref_mag=13.85 +/- 0.04 new_mean_mag=13.7508 delta=0.10 (need > 0.90)
Forced photometry filter REJECTED candidate at 04:21:31.37 +14:25:58.4: ref_mag=13.91 +/- 0.03 new_mean_mag=13.7307 delta=0.18 (need > 0.90)
Forced photometry reference-image weighted average: 13.67 +/- 0.03
Forced photometry filter REJECTED candidate at 04:35:39.12 +16:08:31.9: ref_mag=13.67 +/- 0.03 new_mean_mag=13.5377 delta=0.13 (need > 0.90)
Forced photometry reference-image weighted average: 13.93 +/- 0.04
Forced photometry filter REJECTED candidate at 04:25:38.54 +17:55:22.4: ref_mag=13.93 +/- 0.04 new_mean_mag=13.8575 delta=0.07 (need > 0.90)
Forced photometry on wcs_Tau-06-Q1b1x1_2026-02-11_22-19-16_20.00sec_-15.00C_LIGHT_0147.fits at 04:37:05.84 +15:55:35.0: 14.10 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.09 +/- 0.04
Forced photometry filter REJECTED candidate at 04:37:05.84 +15:55:35.0: ref_mag=14.09 +/- 0.04 new_mean_mag=13.9179 delta=0.17 (need > 0.90)
Adding exclusion_list_local.txt__out76404.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out76593.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
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 75636_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375
The candidate 75636_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375 did not pass the final checks
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Considering the candidate 75819_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375
The candidate 75819_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375 did not pass the final checks
**** FOUND 04:26:24.85 +15:35:07.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75923_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375
The candidate 75923_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375 did not pass the final checks
**** FOUND 04:56:12.06 +13:30:59.8 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 75988_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375
The candidate 75988_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375 did not pass the final checks
**** FOUND 04:10:47.90 +18:26:18.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 76172_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375
The candidate 76172_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375 did not pass the final checks
**** FOUND 04:33:58.41 +10:13:54.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 76176_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375
The candidate 76176_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375 did not pass the final checks
**** FOUND 04:21:59.63 +14:06:13.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 76229_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375
The candidate 76229_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375 did not pass the final checks
**** FOUND 04:00:49.55 +12:30:10.3 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 76236_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375
The candidate 76236_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375 did not pass the final checks
**** FOUND 04:30:08.27 +15:39:57.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 76282_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375
The candidate 76282_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375 did not pass the final checks
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Considering the candidate 76297_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375
The candidate 76297_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375 did not pass the final checks
**** FOUND 04:20:48.74 +13:50:48.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 76328_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375
The candidate 76328_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375 did not pass the final checks
**** FOUND 04:30:13.67 +15:39:27.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 76329_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375
The candidate 76329_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375 did not pass the final checks
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Considering the candidate 76375_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375
The candidate 76375_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375 did not pass the final checks
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Considering the candidate 76404_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 76404_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 76407_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375
The candidate 76407_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375 did not pass the final checks
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Considering the candidate 76442_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375
The candidate 76442_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375 did not pass the final checks
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Considering the candidate 76522_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375
The candidate 76522_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375 did not pass the final checks
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Considering the candidate 76593_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375
Preparing report for the candidate 76593_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375
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Considering the candidate 76607_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375
The candidate 76607_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375 did not pass the final checks
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Considering the candidate 54361_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375
The candidate 54361_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375 did not pass the final checks
**** FOUND 04:54:18.50 +11:10:44.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 36294_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375
The candidate 36294_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375 did not pass the final checks
**** FOUND 04:55:05.60 +13:07:35.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56370_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375
The candidate 56370_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375 did not pass the final checks
**** FOUND 04:43:23.98 +11:35:05.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 09875_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375
The candidate 09875_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375 did not pass the final checks
**** FOUND 04:52:02.18 +17:32:15.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 05737_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375
The candidate 05737_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375 did not pass the final checks
**** FOUND 04:17:46.00 +18:22:35.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 39342_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375
The candidate 39342_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375 did not pass the final checks
**** FOUND 04:50:36.68 +08:53:58.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 47885_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375
The candidate 47885_fd_Tau-06-Q1b1x1_2026-08-18_03-49-21_20.00sec_-0.00C_LIGHTs_0375 did not pass the final checks