This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO
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 09 14.3563 2461297.8563 13.92 03:17:12.07 +10:53:14.7
170.76324 -38.09419 galactic Ari Second-epoch detections are separated by 0.8" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.619 Triberga 0 0 0 13.9 -0 0
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:17:12.07 +10:53:14.7: 16.17 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:17:12.07 +10:53:14.7: 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 09 14.3563* 03 17 12.07 +10 53 14.7 13.9 U Ari 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461297.8563,13.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260914.3563 13.92CV 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 09 14.3563 2461297.8563 14.39 03:49:07.26 +17:01:37.8
172.41108 -28.31118 galactic Tau Second-epoch detections are separated by 1.3" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.131 Vala -1 0 1 14.7 -0 -0
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:49:07.26 +17:01:37.8: 16.15 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:49:07.26 +17:01:37.8: 16.17 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 14.3563* 03 49 07.26 +17 01 37.8 14.4 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,2461297.8563,14.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260914.3563 14.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.67169814 09.01.2026 04:07:04.719 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
First image: 2461049.67169814 09.01.2026 04:07:04.719 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
Last image: 2461297.85671321 14.09.2026 08:33:30.021 /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.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.: -7.43
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 7172
Objects passed selection criteria: 7148
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 5557
Average stars matched: 5091.25 (91.6187 %)
Memory usage VmPeak: 232820 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Sep 11 14:55:52 CDT 2026
VaST build number 1.0rc89-210-g97d43bca
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Sep 14 03:43:11 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.67169814 09.01.2026 04:07:04.719 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
First image: 2461049.67169814 09.01.2026 04:07:04.719 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
Last image: 2461297.85671321 14.09.2026 08:33:30.021 /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 35
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.10
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: 17 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): 45446
Objects passed selection criteria: 45300
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 3.0 2 4
Average stars detected per image: 36279.8
Average stars matched: 33154 (91.3843 %)
Memory usage VmPeak: 262472 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Sep 11 14:55:52 CDT 2026
VaST build number 1.0rc89-210-g97d43bca
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Sep 14 03:44:07 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits
SExtractor catalog cache: saved Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.cat to cache
SExtractor catalog cache: saved Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.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: 2461297.85593854
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits exists and is non-empty
wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits exists and is non-empty
wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits exists and is non-empty
wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits (1st reference image)
verification OK: wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 03:33:20.383 +13:59:53.59 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits (1st new image)
verification OK: wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 03:33:21.549 +14:00:43.07 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 03:33:20.383 +13:59:53.59
Second-epoch image center 03:33:21.549 +14:00:43.07
Angular distance between the image centers 0.0145 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits (2nd new image)
verification OK: wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 03:33:18.884 +14:00:34.33 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 03:33:20.383 +13:59:53.59
Second-epoch image center 03:33:18.884 +14:00:34.33
Angular distance between the image centers 0.0128 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 03:33:21.549 +14:00:43.07
Second-epoch second image center 03:33:18.884 +14:00:34.33
Angular distance between the image centers 0.01104 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits &> /tmp/tmp.GKOGAOB6Ai
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits &> /tmp/tmp.XXWcPzGGvv
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits &> /tmp/tmp.MXzzeHoXY5
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits &> /tmp/tmp.Xw0geFoZOz
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits and wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits and wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat
Found non-empty wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits and wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat
The reference image (wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits) and catalog (wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat) found
'wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat' -> 'wcsmag.cat'
Read 7716 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 45.0636 to 61.6428 deg, Dec +8.6205 to +19.2872 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 45.0636 to 61.6428 deg, Dec 8.6205 to 19.2872 deg
Loaded 4361 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3534 out of 3742 total matches.
Matched with Tycho-2 3742 out of 7716 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.950750
a=0.000000 b=1.000000 c=22.950750
From vast_summary.log: estimated ref. image limiting mag.: -7.43
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.52
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.52
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 7716 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 45.0636 to 61.6428 deg, Dec +8.6205 to +19.2872 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 45.0636 to 61.6428 deg, Dec 8.6205 to 19.2872 deg
Loaded 4361 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3534 out of 3742 total matches.
Matched with Tycho-2 3742 out of 7716 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
Forced-photometry filter: calibrated wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits -> calib.txt_param_ref_wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits (aperture=6.0)
Read 7722 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 45.0650 to 61.6427 deg, Dec +8.6182 to +19.2791 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 45.0650 to 61.6427 deg, Dec 8.6182 to 19.2791 deg
Loaded 4354 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3534 out of 3736 total matches.
Matched with Tycho-2 3736 out of 7722 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
Forced-photometry filter: calibrated wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits -> calib.txt_param_ref_wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits (aperture=6.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
2.0 pix Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
2.3 pix fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits
2.3 pix fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits
Limiting magnitude estimates:
15.5 mag. Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
15.5 mag. Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
15.3 mag. fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits
15.3 mag. fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits
All-image limiting magnitude estimate: 15.3 (SNR ) 12.2 (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.GKOGAOB6Ai (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits' -> 'wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
WCS_IMAGE_NAME=wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
WCS-calibrated image found: wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
Checking if the catalog wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat corresponding to the image wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits alredy exist and is non-empty...
Catalog wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat corresponding to the image wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
WCS catalog name: wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=551, bad_region=1716, passed=7716
Got 7716 stars (including 5573 good ones) from the SExtractor catalog wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat
util/solve_plate_with_UCAC5 got 7716 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4903 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4894 matched stars entering correct_measured_positions(), 4894 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4894 matched stars entering correct_measured_positions(), 6339 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4903 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4894 matched stars entering correct_measured_positions(), 6339 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4894 matched stars entering correct_measured_positions(), 6339 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 4894 stars left (next iteration limit 5383)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits N_match=4894 sigma_overall_arcsec=0.317 sigma_q1_arcsec=0.399 sigma_q2_arcsec=0.313 sigma_q3_arcsec=0.271 sigma_q4_arcsec=0.268 n_q1=1724 n_q2=1005 n_q3=1514 n_q4=651 worst_quadrant_to_overall_ratio=1.261
The image catalog is written to wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits -region wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.XXWcPzGGvv (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits' -> 'wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
WCS_IMAGE_NAME=wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
WCS-calibrated image found: wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
Checking if the catalog wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat corresponding to the image wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits alredy exist and is non-empty...
Catalog wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat corresponding to the image wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
WCS catalog name: wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=536, bad_region=1716, passed=7722
Got 7722 stars (including 5589 good ones) from the SExtractor catalog wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat
util/solve_plate_with_UCAC5 got 7722 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4905 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4897 matched stars entering correct_measured_positions(), 4897 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4897 matched stars entering correct_measured_positions(), 6342 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4905 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4898 matched stars entering correct_measured_positions(), 6342 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4898 matched stars entering correct_measured_positions(), 6342 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4898 stars left (next iteration limit 5386)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits N_match=4898 sigma_overall_arcsec=0.324 sigma_q1_arcsec=0.409 sigma_q2_arcsec=0.297 sigma_q3_arcsec=0.276 sigma_q4_arcsec=0.273 n_q1=1731 n_q2=1006 n_q3=1513 n_q4=648 worst_quadrant_to_overall_ratio=1.264
The image catalog is written to wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits -region wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.MXzzeHoXY5 (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_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.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_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits
WCS_IMAGE_NAME=wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits
WCS-calibrated image found: wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits
Checking if the catalog wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits.wcscat corresponding to the image wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits.wcscat corresponding to the image wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits
WCS catalog name: wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=402, bad_region=1780, passed=6952
Got 6952 stars (including 4846 good ones) from the SExtractor catalog wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits.wcscat
util/solve_plate_with_UCAC5 got 6952 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4749 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4740 matched stars entering correct_measured_positions(), 4741 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4740 matched stars entering correct_measured_positions(), 5536 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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4751 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4742 matched stars entering correct_measured_positions(), 5536 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4742 matched stars entering correct_measured_positions(), 5536 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 4742 stars left (next iteration limit 5214)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4742 robust_rms=7.305 arcsec worst_quadrant_rms=11.031 arcsec
SIP_REFIT: SIP order 3 trial: matched=4742 robust_rms=0.479 arcsec worst_quadrant_rms=0.601 arcsec
SIP_REFIT: SIP order 5 trial: matched=4742 robust_rms=0.361 arcsec worst_quadrant_rms=0.398 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4742 robust_rms_before=1.035 arcsec robust_rms_before_corrected=0.372 arcsec robust_rms_after=0.361 arcsec worst_quadrant_rms_before=0.415 worst_quadrant_rms_after=0.398
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.415 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits N_match=4742 sigma_overall_arcsec=0.392 sigma_q1_arcsec=0.343 sigma_q2_arcsec=0.404 sigma_q3_arcsec=0.446 sigma_q4_arcsec=0.364 n_q1=1225 n_q2=801 n_q3=1702 n_q4=1014 worst_quadrant_to_overall_ratio=1.138
The image catalog is written to wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits -region wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.Xw0geFoZOz (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_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.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_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits
WCS_IMAGE_NAME=wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits
WCS-calibrated image found: wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits
Checking if the catalog wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits.wcscat corresponding to the image wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits.wcscat corresponding to the image wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits
WCS catalog name: wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=413, bad_region=1801, passed=6974
Got 6974 stars (including 4843 good ones) from the SExtractor catalog wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits.wcscat
util/solve_plate_with_UCAC5 got 6974 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4745 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4736 matched stars entering correct_measured_positions(), 4736 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4736 matched stars entering correct_measured_positions(), 5540 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 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4745 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4735 matched stars entering correct_measured_positions(), 5540 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 4735 matched stars entering correct_measured_positions(), 5540 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 4735 stars left (next iteration limit 5209)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4735 robust_rms=7.244 arcsec worst_quadrant_rms=11.201 arcsec
SIP_REFIT: SIP order 3 trial: matched=4735 robust_rms=0.472 arcsec worst_quadrant_rms=0.583 arcsec
SIP_REFIT: SIP order 5 trial: matched=4735 robust_rms=0.368 arcsec worst_quadrant_rms=0.389 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4735 robust_rms_before=1.028 arcsec robust_rms_before_corrected=0.374 arcsec robust_rms_after=0.368 arcsec worst_quadrant_rms_before=0.398 worst_quadrant_rms_after=0.389
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.398 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits N_match=4735 sigma_overall_arcsec=0.401 sigma_q1_arcsec=0.340 sigma_q2_arcsec=0.411 sigma_q3_arcsec=0.443 sigma_q4_arcsec=0.384 n_q1=1209 n_q2=803 n_q3=1702 n_q4=1021 worst_quadrant_to_overall_ratio=1.104
The image catalog is written to wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits -region wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits to local_wcs_cache/
'wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits' -> 'local_wcs_cache/wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits'
Saving the final (post-refit) wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits to local_wcs_cache/
'wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits' -> 'local_wcs_cache/wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits'
Saving the final (post-refit) wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits to local_wcs_cache/
'wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits' -> 'local_wcs_cache/wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits'
Saving the final (post-refit) wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits to local_wcs_cache/
'wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits' -> 'local_wcs_cache/wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits sigma_overall=0.317 worst_q_ratio=1.261
ref2=Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits sigma_overall=0.324 worst_q_ratio=1.264
new1=fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits sigma_overall=0.392 worst_q_ratio=1.138
new2=fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits sigma_overall=0.401 worst_q_ratio=1.104
reference average sigma_overall=0.3205 worst_q_ratio=1.2625
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137_astrometric_residuals.png (4894 matched stars from wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138_astrometric_residuals.png (4898 matched stars from wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434_astrometric_residuals.png (4742 matched stars from wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435_astrometric_residuals.png (4735 matched stars from wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits'
Saving fully-calibrated image wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits'
Preparing the HTML report for the field Tau-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:25:43.77 +17:25:56.7: 11.77 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:38:10.31 +13:46:02.4: 12.47 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:43:26.68 +12:49:58.2: 12.37 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:25:43.77 +17:25:56.7: 11.76 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:38:10.31 +13:46:02.4: 12.47 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:43:26.68 +12:49:58.2: 12.36 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.76 +/- 0.00
Forced photometry reference-image weighted average: 12.47 +/- 0.01
Forced photometry filter REJECTED candidate at 03:25:43.77 +17:25:56.7: ref_mag=11.76 +/- 0.00 new_mean_mag=12.2009 delta=-0.44 (need > 0.90)
Forced photometry reference-image weighted average: 12.36 +/- 0.01
Forced photometry filter REJECTED candidate at 03:38:10.31 +13:46:02.4: ref_mag=12.47 +/- 0.01 new_mean_mag=12.4451 delta=0.02 (need > 0.90)
Forced photometry filter REJECTED candidate at 03:43:26.68 +12:49:58.2: ref_mag=12.36 +/- 0.01 new_mean_mag=12.3636 delta=0.00 (need > 0.90)
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 20315_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435
The candidate 20315_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21477_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435
The candidate 21477_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21533_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435
The candidate 21533_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435 did not pass the final checks
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-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits
SExtractor catalog cache: saved Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.cat to cache
SExtractor catalog cache: saved Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
Creating symlink local_wcs_cache/wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits exists and is non-empty
wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits exists and is non-empty
wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits exists and is non-empty
wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits (1st reference image)
verification OK: wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 03:33:20.383 +13:59:53.59 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits (1st new image)
verification OK: wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 03:33:21.549 +14:00:43.07 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 03:33:20.383 +13:59:53.59
Second-epoch image center 03:33:21.549 +14:00:43.07
Angular distance between the image centers 0.0145 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits (2nd new image)
verification OK: wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 03:33:18.884 +14:00:34.33 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 03:33:20.383 +13:59:53.59
Second-epoch image center 03:33:18.884 +14:00:34.33
Angular distance between the image centers 0.0128 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 03:33:21.549 +14:00:43.07
Second-epoch second image center 03:33:18.884 +14:00:34.33
Angular distance between the image centers 0.01104 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits &> /tmp/tmp.zjLzZNd7ZL
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits &> /tmp/tmp.Uc7vzwocjQ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits &> /tmp/tmp.NDAb9AM7Ev
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits &> /tmp/tmp.HuZV3KI7Tt
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits and wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits and wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat
Found non-empty wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits and wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat
The reference image (wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits) and catalog (wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat) found
'wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat' -> 'wcsmag.cat'
Read 48584 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 45.0636 to 61.6458 deg, Dec +8.6191 to +19.2871 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 45.0636 to 61.6458 deg, Dec 8.6191 to 19.2871 deg
Loaded 4361 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3309 out of 3760 total matches.
Matched with Tycho-2 3760 out of 48584 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.817800
a=0.000000 b=1.000000 c=22.817800
From vast_summary.log: estimated ref. image limiting mag.: -7.10
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.72
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.72
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 48584 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 45.0636 to 61.6458 deg, Dec +8.6191 to +19.2871 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 45.0636 to 61.6458 deg, Dec 8.6191 to 19.2871 deg
Loaded 4361 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3309 out of 3760 total matches.
Matched with Tycho-2 3760 out of 48584 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
Forced-photometry filter: calibrated wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits -> calib.txt_param_ref_wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits (aperture=4.5)
Read 48560 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 45.0650 to 61.6548 deg, Dec +8.6183 to +19.2794 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 45.0650 to 61.6548 deg, Dec 8.6183 to 19.2794 deg
Loaded 4358 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3320 out of 3753 total matches.
Matched with Tycho-2 3753 out of 48560 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
Forced-photometry filter: calibrated wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits -> calib.txt_param_ref_wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits (aperture=4.6)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 23 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
1.9 pix Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
2.1 pix fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits
2.1 pix fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits
Limiting magnitude estimates:
15.7 mag. Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
15.7 mag. Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
15.5 mag. fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits
15.5 mag. fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits
All-image limiting magnitude estimate: 15.5 (SNR ) 14.8 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.zjLzZNd7ZL (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits' -> 'wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
WCS_IMAGE_NAME=wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
WCS-calibrated image found: wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
Checking if the catalog wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat corresponding to the image wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits alredy exist and is non-empty...
Catalog wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat corresponding to the image wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits
WCS catalog name: wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=2222, bad_region=8835, passed=48571
Got 48571 stars (including 37859 good ones) from the SExtractor catalog wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat
util/solve_plate_with_UCAC5 got 48571 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4899 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4893 matched stars entering correct_measured_positions(), 4893 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4893 matched stars entering correct_measured_positions(), 41607 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4899 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4893 matched stars entering correct_measured_positions(), 41607 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 4893 matched stars entering correct_measured_positions(), 41607 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4893 stars left (next iteration limit 5382)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits N_match=4893 sigma_overall_arcsec=0.310 sigma_q1_arcsec=0.385 sigma_q2_arcsec=0.297 sigma_q3_arcsec=0.269 sigma_q4_arcsec=0.268 n_q1=1704 n_q2=988 n_q3=1521 n_q4=680 worst_quadrant_to_overall_ratio=1.244
The image catalog is written to wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits -region wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.Uc7vzwocjQ (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits' -> 'wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
WCS_IMAGE_NAME=wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
WCS-calibrated image found: wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
Checking if the catalog wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat corresponding to the image wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits alredy exist and is non-empty...
Catalog wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat corresponding to the image wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits
WCS catalog name: wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=2192, bad_region=8846, passed=48544
Got 48544 stars (including 37859 good ones) from the SExtractor catalog wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat
util/solve_plate_with_UCAC5 got 48544 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4897 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4890 matched stars entering correct_measured_positions(), 4890 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4890 matched stars entering correct_measured_positions(), 41566 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4897 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4891 matched stars entering correct_measured_positions(), 41566 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 4891 matched stars entering correct_measured_positions(), 41566 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4891 stars left (next iteration limit 5379)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits N_match=4891 sigma_overall_arcsec=0.310 sigma_q1_arcsec=0.392 sigma_q2_arcsec=0.285 sigma_q3_arcsec=0.263 sigma_q4_arcsec=0.271 n_q1=1699 n_q2=994 n_q3=1515 n_q4=683 worst_quadrant_to_overall_ratio=1.265
The image catalog is written to wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits -region wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.NDAb9AM7Ev (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_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.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_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits
WCS_IMAGE_NAME=wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits
WCS-calibrated image found: wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits
Checking if the catalog wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits.wcscat corresponding to the image wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits.wcscat corresponding to the image wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits
WCS catalog name: wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=1833, bad_region=8175, passed=41356
Got 41356 stars (including 31832 good ones) from the SExtractor catalog wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits.wcscat
util/solve_plate_with_UCAC5 got 41356 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4889 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4880 matched stars entering correct_measured_positions(), 4880 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4880 matched stars entering correct_measured_positions(), 35171 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4888 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4880 matched stars entering correct_measured_positions(), 35171 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 4880 matched stars entering correct_measured_positions(), 35171 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 4880 stars left (next iteration limit 5368)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.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=4880 robust_rms=7.082 arcsec worst_quadrant_rms=9.841 arcsec
SIP_REFIT: SIP order 3 trial: matched=4880 robust_rms=0.473 arcsec worst_quadrant_rms=0.596 arcsec
SIP_REFIT: SIP order 5 trial: matched=4880 robust_rms=0.358 arcsec worst_quadrant_rms=0.401 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4880 robust_rms_before=1.014 arcsec robust_rms_before_corrected=0.366 arcsec robust_rms_after=0.358 arcsec worst_quadrant_rms_before=0.411 worst_quadrant_rms_after=0.401
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.411 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits N_match=4880 sigma_overall_arcsec=0.388 sigma_q1_arcsec=0.345 sigma_q2_arcsec=0.392 sigma_q3_arcsec=0.446 sigma_q4_arcsec=0.357 n_q1=1306 n_q2=801 n_q3=1703 n_q4=1070 worst_quadrant_to_overall_ratio=1.149
The image catalog is written to wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits -region wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.HuZV3KI7Tt (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_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.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_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits
WCS_IMAGE_NAME=wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits
WCS-calibrated image found: wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits
Checking if the catalog wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits.wcscat corresponding to the image wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits.wcscat corresponding to the image wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits
WCS catalog name: wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=1813, bad_region=8239, passed=41531
Got 41531 stars (including 31934 good ones) from the SExtractor catalog wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits.wcscat
util/solve_plate_with_UCAC5 got 41531 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 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: 4881 matched stars entering correct_measured_positions(), 4882 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4881 matched stars entering correct_measured_positions(), 35296 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 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(), 35296 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 4881 matched stars entering correct_measured_positions(), 35296 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 4881 stars left (next iteration limit 5369)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.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=4881 robust_rms=7.043 arcsec worst_quadrant_rms=9.420 arcsec
SIP_REFIT: SIP order 3 trial: matched=4881 robust_rms=0.461 arcsec worst_quadrant_rms=0.570 arcsec
SIP_REFIT: SIP order 5 trial: matched=4881 robust_rms=0.367 arcsec worst_quadrant_rms=0.394 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4881 robust_rms_before=1.005 arcsec robust_rms_before_corrected=0.380 arcsec robust_rms_after=0.367 arcsec worst_quadrant_rms_before=0.409 worst_quadrant_rms_after=0.394
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.409 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits N_match=4881 sigma_overall_arcsec=0.397 sigma_q1_arcsec=0.343 sigma_q2_arcsec=0.408 sigma_q3_arcsec=0.441 sigma_q4_arcsec=0.377 n_q1=1295 n_q2=800 n_q3=1711 n_q4=1075 worst_quadrant_to_overall_ratio=1.110
The image catalog is written to wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits -region wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.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_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-32-23_20.00sec_-0.00C_LIGHT_0434.fits
Saving fully-calibrated image wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.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_2026-09-14_CI_Tau-05-Q2b1x1_034055_TTUQ2b1x1_2140696_WWl2u8OO/wcs_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435.fits
Preparing the HTML report for the field Tau-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:32:32.74 +15:13:12.1: 12.50 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:49:07.26 +17:01:37.8: 16.15 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:45:33.56 +12:52:25.2: 14.40 +/- 0.07 detection
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:33:53.52 +18:14:08.6: 14.37 +/- 0.09 detection
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:37:52.05 +10:46:42.7: 14.52 +/- 0.09 detection
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:28:24.24 +15:51:21.8: 14.34 +/- 0.06 detection
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:34:18.73 +10:38:18.8: 14.55 +/- 0.08 detection
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:23:30.55 +17:10:28.0: 14.43 +/- 0.08 detection
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:17:12.07 +10:53:14.7: 16.17 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:43:23.81 +18:09:01.5: 14.56 +/- 0.08 detection
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:37:52.05 +10:46:42.7: 14.60 +/- 0.09 detection
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:28:24.24 +15:51:21.8: 14.22 +/- 0.05 detection
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:32:32.74 +15:13:12.1: 12.54 +/- 0.01 detection
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:23:30.55 +17:10:28.0: 14.39 +/- 0.07 detection
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:33:53.52 +18:14:08.6: 14.28 +/- 0.08 detection
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:17:12.07 +10:53:14.7: 16.13 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:45:33.56 +12:52:25.2: 14.36 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.28 +/- 0.04
Forced photometry reference-image weighted average: 12.52 +/- 0.01
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:49:07.26 +17:01:37.8: 16.17 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 14.55 +/- 0.06
Forced photometry filter REJECTED candidate at 03:28:24.24 +15:51:21.8: ref_mag=14.28 +/- 0.04 new_mean_mag=14.5184 delta=-0.24 (need > 0.90)
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:34:18.73 +10:38:18.8: 14.45 +/- 0.07 detection
Forced photometry filter REJECTED candidate at 03:32:32.74 +15:13:12.1: ref_mag=12.52 +/- 0.01 new_mean_mag=12.6795 delta=-0.16 (need > 0.90)
Forced photometry reference-image weighted average: 14.41 +/- 0.05
Forced photometry filter REJECTED candidate at 03:37:52.05 +10:46:42.7: ref_mag=14.55 +/- 0.06 new_mean_mag=14.7013 delta=-0.15 (need > 0.90)
Forced photometry reference-image weighted average: 14.38 +/- 0.05
Forced photometry filter REJECTED candidate at 03:23:30.55 +17:10:28.0: ref_mag=14.41 +/- 0.05 new_mean_mag=14.4439 delta=-0.03 (need > 0.90)
Forced photometry reference-image weighted average: 14.32 +/- 0.06
Forced photometry filter REJECTED candidate at 03:45:33.56 +12:52:25.2: ref_mag=14.38 +/- 0.05 new_mean_mag=14.4623 delta=-0.08 (need > 0.90)
Forced photometry filter REJECTED candidate at 03:33:53.52 +18:14:08.6: ref_mag=14.32 +/- 0.06 new_mean_mag=14.5643 delta=-0.25 (need > 0.90)
Forced photometry reference-image weighted average: 14.49 +/- 0.05
Forced photometry filter REJECTED candidate at 03:34:18.73 +10:38:18.8: ref_mag=14.49 +/- 0.05 new_mean_mag=14.5605 delta=-0.07 (need > 0.90)
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:43:23.81 +18:09:01.5: 14.72 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.63 +/- 0.06
Forced photometry filter REJECTED candidate at 03:43:23.81 +18:09:01.5: ref_mag=14.63 +/- 0.06 new_mean_mag=14.6577 delta=-0.03 (need > 0.90)
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:22:30.17 +13:43:05.9: 15.50 +/- 0.18 detection
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:26:01.01 +09:58:06.4: 15.66 +/- 0.23 detection
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:16:55.07 +15:15:06.1: 15.28 +/- 0.16 detection
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:17:48.38 +17:50:35.7: 15.01 +/- 0.13 detection
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:20:36.60 +14:40:18.2: 14.78 +/- 0.10 detection
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:31:49.56 +15:08:04.5: 15.10 +/- 0.12 detection
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:19:03.76 +10:35:00.0: 15.65 +/- 0.21 detection
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:18:30.73 +09:56:31.6: 15.09 +/- 0.14 detection
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:22:30.17 +13:43:05.9: 15.54 +/- 0.20 detection
Forced photometry reference-image weighted average: 15.52 +/- 0.13
Forced photometry filter REJECTED candidate at 03:22:30.17 +13:43:05.9: ref_mag=15.52 +/- 0.13 new_mean_mag=15.1492 delta=0.37 (need > 0.90)
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:26:01.01 +09:58:06.4: 15.72 +/- 0.24 detection
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:31:49.56 +15:08:04.5: 14.94 +/- 0.11 detection
Forced photometry reference-image weighted average: 15.69 +/- 0.17
Forced photometry filter REJECTED candidate at 03:26:01.01 +09:58:06.4: ref_mag=15.69 +/- 0.17 new_mean_mag=15.0537 delta=0.63 (need > 0.90)
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:16:55.07 +15:15:06.1: 15.35 +/- 0.17 detection
Forced photometry reference-image weighted average: 15.01 +/- 0.08
Forced photometry filter REJECTED candidate at 03:31:49.56 +15:08:04.5: ref_mag=15.01 +/- 0.08 new_mean_mag=14.7397 delta=0.27 (need > 0.90)
Forced photometry reference-image weighted average: 15.31 +/- 0.12
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:17:48.38 +17:50:35.7: 15.18 +/- 0.15 detection
Forced photometry filter REJECTED candidate at 03:16:55.07 +15:15:06.1: ref_mag=15.31 +/- 0.12 new_mean_mag=15.1593 delta=0.15 (need > 0.90)
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:20:36.60 +14:40:18.2: 14.50 +/- 0.07 detection
Forced photometry reference-image weighted average: 15.08 +/- 0.10
Forced photometry filter REJECTED candidate at 03:17:48.38 +17:50:35.7: ref_mag=15.08 +/- 0.10 new_mean_mag=15.0563 delta=0.03 (need > 0.90)
Forced photometry reference-image weighted average: 14.60 +/- 0.06
Forced photometry filter REJECTED candidate at 03:20:36.60 +14:40:18.2: ref_mag=14.60 +/- 0.06 new_mean_mag=14.7201 delta=-0.12 (need > 0.90)
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:19:03.76 +10:35:00.0: 15.28 +/- 0.16 detection
Forced photometry reference-image weighted average: 15.42 +/- 0.13
Forced photometry filter REJECTED candidate at 03:19:03.76 +10:35:00.0: ref_mag=15.42 +/- 0.13 new_mean_mag=15.1192 delta=0.30 (need > 0.90)
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:18:30.73 +09:56:31.6: 15.36 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.19 +/- 0.11
Forced photometry filter REJECTED candidate at 03:18:30.73 +09:56:31.6: ref_mag=15.19 +/- 0.11 new_mean_mag=15.1829 delta=0.00 (need > 0.90)
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:49:03.73 +17:02:59.7: 15.24 +/- 0.15 detection
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:46:50.03 +17:10:46.8: 15.62 +/- 0.21 detection
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:21:57.96 +12:44:48.4: 15.47 +/- 0.17 detection
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-07-04_20.00sec_-14.90C_LIGHT_0137.fits at 03:15:44.06 +15:31:06.2: 15.14 +/- 0.14 detection
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:49:03.73 +17:02:59.7: 15.54 +/- 0.20 detection
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:46:50.03 +17:10:46.8: 16.12 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:15:44.06 +15:31:06.2: 14.83 +/- 0.11 detection
Forced photometry reference-image weighted average: 15.62 +/- 0.21
Forced photometry reference-image weighted average: 15.35 +/- 0.12
Forced photometry filter REJECTED candidate at 03:46:50.03 +17:10:46.8: ref_mag=15.62 +/- 0.21 new_mean_mag=15.1968 delta=0.43 (need > 0.90)
Forced photometry filter REJECTED candidate at 03:49:03.73 +17:02:59.7: ref_mag=15.35 +/- 0.12 new_mean_mag=15.1203 delta=0.23 (need > 0.90)
Forced photometry reference-image weighted average: 14.94 +/- 0.09
Forced photometry filter REJECTED candidate at 03:15:44.06 +15:31:06.2: ref_mag=14.94 +/- 0.09 new_mean_mag=14.8954 delta=0.05 (need > 0.90)
Forced photometry on wcs_Tau-05-Q2b1x1_2026-01-08_22-08-02_20.00sec_-14.90C_LIGHT_0138.fits at 03:21:57.96 +12:44:48.4: 15.61 +/- 0.21 detection
Forced photometry reference-image weighted average: 15.53 +/- 0.13
Forced photometry filter REJECTED candidate at 03:21:57.96 +12:44:48.4: ref_mag=15.53 +/- 0.13 new_mean_mag=15.2000 delta=0.33 (need > 0.90)
Adding exclusion_list_local.txt__out56493.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out58244.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 52909_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435
The candidate 52909_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435 did not pass the final checks
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Considering the candidate 52913_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435
The candidate 52913_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52915_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435
The candidate 52915_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435 did not pass the final checks
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Considering the candidate 52917_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435
The candidate 52917_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435 did not pass the final checks
**** FOUND 03:28:01.91 +18:05:23.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52918_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435
The candidate 52918_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435 did not pass the final checks
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Considering the candidate 56493_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435
Preparing report for the candidate 56493_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435
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Considering the candidate 58170_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435
The candidate 58170_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435 did not pass the final checks
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Considering the candidate 58244_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435
Preparing report for the candidate 58244_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435
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Considering the candidate 58587_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435
The candidate 58587_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435 did not pass the final checks
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Considering the candidate 58665_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435
The candidate 58665_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435 did not pass the final checks
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Considering the candidate 59042_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435
The candidate 59042_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435 did not pass the final checks
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Considering the candidate 59457_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435
The candidate 59457_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435 did not pass the final checks
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Considering the candidate 59461_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435
The candidate 59461_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435 did not pass the final checks
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Considering the candidate 59906_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435
The candidate 59906_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435 did not pass the final checks
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Considering the candidate 60239_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435
The candidate 60239_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435 did not pass the final checks
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Considering the candidate 60262_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435
The candidate 60262_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435 did not pass the final checks
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Considering the candidate 60292_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435
The candidate 60292_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435 did not pass the final checks
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Considering the candidate 60316_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435
The candidate 60316_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435 did not pass the final checks
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Considering the candidate 60401_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435
The candidate 60401_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435 did not pass the final checks
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Considering the candidate 60426_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435
The candidate 60426_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435 did not pass the final checks
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Considering the candidate 60445_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435
The candidate 60445_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435 did not pass the final checks
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Considering the candidate 60493_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435
The candidate 60493_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435 did not pass the final checks
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Considering the candidate 60527_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435
The candidate 60527_fd_Tau-05-Q2b1x1_2026-09-14_03-33-30_20.00sec_-0.00C_LIGHT_0435 did not pass the final checks