This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP
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 07 28.3877 2461249.8877 13.09 04:39:30.61 +21:51:21.2
177.12243 -16.25501 galactic Tau Second-epoch detections are separated by 2.6" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.110 Lydia 0 -1 1 13.4 0 0
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:39:30.61 +21:51:21.2: 16.40 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits at 04:39:30.61 +21:51:21.2: 16.37 +/- 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 07 28.3877* 04 39 30.61 +21 51 21.2 13.1 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,2461249.8877,13.09,0.05,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 20260728.3877 13.09CV 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 07 28.3877 2461249.8877 12.13 04:44:21.54 +22:50:07.3
177.05756 -14.76758 galactic Tau Second-epoch detections are separated by 0.9" and 7.1 pix
The object was found in VSX 2" ASAS J044422+2250.2
Type: SR
# Max. Min./Amp. JD0 Period
8.778 Ic Y 0.287 Ic 2453201.80000 355.000000000000
The object was not found in astcheck.
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:44:21.54 +22:50:07.3: 13.08 +/- 0.02 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits at 04:44:21.54 +22:50:07.3: 13.11 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.01
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 07 28.3877* 04 44 21.54 +22 50 07.3 12.1 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
ASAS J044422+2250.2,2461249.8877,12.13,0.05,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
ASAS J044422+2250.2 20260728.3877 12.13CV 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: 2461049.68987713 09.01.2026 04:33:15.384 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
First image: 2461049.68987713 09.01.2026 04:33:15.384 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Last image: 2461249.88798337 28.07.2026 09:18:31.763 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.49
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: 5 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
Total objects detected (at least 2 times): 9358
Objects passed selection criteria: 9289
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 5636.5
Average stars matched: 5333.5 (94.6243 %)
Memory usage VmPeak: 235728 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Jul 28 02:13:30 CDT 2026
VaST build number 1.0rc89-182-g8380f0ac
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-28)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Jul 28 06:29:42 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: 2461049.68987713 09.01.2026 04:33:15.384 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
First image: 2461049.68987713 09.01.2026 04:33:15.384 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Last image: 2461249.88798337 28.07.2026 09:18:31.763 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 16
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.17
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 16 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 69265
Objects passed selection criteria: 69040
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 43479.5
Average stars matched: 40884 (94.0305 %)
Memory usage VmPeak: 290664 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Jul 28 02:13:30 CDT 2026
VaST build number 1.0rc89-182-g8380f0ac
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-28)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Jul 28 06:33:49 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-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits
SExtractor catalog cache: saved Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.cat to cache
SExtractor catalog cache: saved Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.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-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_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: 2461249.88732259
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-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits exists and is non-empty
Saving wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits to local_wcs_cache/
'wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits' -> 'local_wcs_cache/wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits'
wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits exists and is non-empty
Saving wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits to local_wcs_cache/
'wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits' -> 'local_wcs_cache/wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits'
wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits exists and is non-empty
Saving wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits to local_wcs_cache/
'wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits' -> 'local_wcs_cache/wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits'
wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits exists and is non-empty
Saving wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits to local_wcs_cache/
'wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits' -> 'local_wcs_cache/wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits (1st reference image)
verification OK: wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Image size: 941.4'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 04:36:56.001 +21:59:37.88 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-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits (1st new image)
verification OK: wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits
Image size: 940.9'x624.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 04:36:57.621 +21:57:03.66 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 04:36:56.001 +21:59:37.88
Second-epoch image center 04:36:57.621 +21:57:03.66
Angular distance between the image centers 0.0433 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits (2nd new image)
verification OK: wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits
Image size: 940.8'x624.4' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 04:36:55.689 +21:57:37.14 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 04:36:56.001 +21:59:37.88
Second-epoch image center 04:36:55.689 +21:57:37.14
Angular distance between the image centers 0.0336 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 04:36:57.621 +21:57:03.66
Second-epoch second image center 04:36:55.689 +21:57:37.14
Angular distance between the image centers 0.01193 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-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits &> /tmp/tmp.g1ZwV0y0Ld
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits &> /tmp/tmp.WuuuKu2qts
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits &> /tmp/tmp.UjQ83kixwP
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits &> /tmp/tmp.I8FqkcjDxY
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits and wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits and wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat
Found non-empty wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits and wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat
The reference image (wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits) and catalog (wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat) found
'wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat' -> 'wcsmag.cat'
Read 11927 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 60.5122 to 78.0896 deg, Dec +16.4863 to +27.2832 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 60.5122 to 78.0896 deg, Dec 16.4863 to 27.2832 deg
Loaded 5179 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): 3947 out of 4318 total matches.
Matched with Tycho-2 4318 out of 11927 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.990300
a=0.000000 b=1.000000 c=22.990300
From vast_summary.log: estimated ref. image limiting mag.: -7.49
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.50
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.50
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 11927 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 60.5122 to 78.0896 deg, Dec +16.4863 to +27.2832 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 60.5122 to 78.0896 deg, Dec 16.4863 to 27.2832 deg
Loaded 5179 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): 3947 out of 4318 total matches.
Matched with Tycho-2 4318 out of 11927 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits:
Forced-photometry filter: calibrated wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits -> calib.txt_param_ref_wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits (aperture=5.9)
Read 12023 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 60.5322 to 78.0896 deg, Dec +16.4883 to +27.2799 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 60.5322 to 78.0896 deg, Dec 16.4883 to 27.2799 deg
Loaded 5164 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): 3942 out of 4310 total matches.
Matched with Tycho-2 4310 out of 12023 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits:
Forced-photometry filter: calibrated wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits -> calib.txt_param_ref_wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits (aperture=5.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
2.0 pix Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
2.4 pix fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits
2.4 pix fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits
2.0 pix wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
2.0 pix wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
Limiting magnitude estimates:
15.5 mag. Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
15.5 mag. Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
13.2 mag. fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits
13.2 mag. fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits
All-image limiting magnitude estimate: 13.2 (SNR ) 10.7 (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
############ /tmp/tmp.g1ZwV0y0Ld (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-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits' -> 'wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
WCS_IMAGE_NAME=wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
WCS-calibrated image found: wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Checking if the catalog wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat corresponding to the image wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits alredy exist and is non-empty...
Catalog wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat corresponding to the image wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
WCS catalog name: wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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=967, bad_region=2517, passed=11927
Got 11927 stars (including 8622 good ones) from the SExtractor catalog wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat
util/solve_plate_with_UCAC5 got 11927 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4851 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4821 matched stars entering correct_measured_positions(), 4821 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4821 matched stars entering correct_measured_positions(), 9924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4850 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4820 matched stars entering correct_measured_positions(), 9924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4820 matched stars entering correct_measured_positions(), 9924 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4820 stars left (next iteration limit 5303)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits N_match=4820 sigma_overall_arcsec=0.312 sigma_q1_arcsec=0.397 sigma_q2_arcsec=0.325 sigma_q3_arcsec=0.273 sigma_q4_arcsec=0.257 n_q1=1641 n_q2=611 n_q3=1816 n_q4=752 worst_quadrant_to_overall_ratio=1.271
The image catalog is written to wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits -region wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.WuuuKu2qts (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-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.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_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.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-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.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-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits' -> 'wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.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-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
WCS_IMAGE_NAME=wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
WCS-calibrated image found: wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
Checking if the catalog wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits.wcscat corresponding to the image wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits alredy exist and is non-empty...
Catalog wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits.wcscat corresponding to the image wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
WCS catalog name: wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.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=981, bad_region=2530, passed=12023
Got 12023 stars (including 8694 good ones) from the SExtractor catalog wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits.wcscat
util/solve_plate_with_UCAC5 got 12023 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4852 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4819 matched stars entering correct_measured_positions(), 4820 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4819 matched stars entering correct_measured_positions(), 10006 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4849 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4816 matched stars entering correct_measured_positions(), 10006 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4816 matched stars entering correct_measured_positions(), 10006 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4816 stars left (next iteration limit 5300)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits N_match=4816 sigma_overall_arcsec=0.303 sigma_q1_arcsec=0.406 sigma_q2_arcsec=0.310 sigma_q3_arcsec=0.256 sigma_q4_arcsec=0.235 n_q1=1636 n_q2=613 n_q3=1811 n_q4=756 worst_quadrant_to_overall_ratio=1.338
The image catalog is written to wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits -region wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.UjQ83kixwP (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_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_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_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits
WCS_IMAGE_NAME=wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits
WCS-calibrated image found: wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits
Checking if the catalog wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits.wcscat corresponding to the image wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits.wcscat corresponding to the image wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_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-03-Q2b1x1_2026-07-28_04-17-34_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_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits
WCS catalog name: wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_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=235, bad_region=571, passed=2454
Got 2454 stars (including 1683 good ones) from the SExtractor catalog wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits.wcscat
util/solve_plate_with_UCAC5 got 2454 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.9'
Seting catalog search parameters based on the expected field of view 940.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013068 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010454 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.2)
Done reading UCAC5 zone files...
Matched 1647 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1645 matched stars entering correct_measured_positions(), 1644 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1645 matched stars entering correct_measured_positions(), 1977 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
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 532 to 588 (Dec 16.5 to 27.2)
Done reading UCAC5 zone files...
Matched 1647 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1644 matched stars entering correct_measured_positions(), 1977 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 1644 matched stars entering correct_measured_positions(), 1977 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 1644 stars left (next iteration limit 1809)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=1644 robust_rms=6.183 arcsec worst_quadrant_rms=8.420 arcsec
SIP_REFIT: SIP order 3 trial: matched=1644 robust_rms=0.566 arcsec worst_quadrant_rms=0.676 arcsec
SIP_REFIT: SIP order 5 trial: matched=1644 robust_rms=0.486 arcsec worst_quadrant_rms=0.507 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=1644 robust_rms_before=1.703 arcsec robust_rms_before_corrected=0.523 arcsec robust_rms_after=0.486 arcsec worst_quadrant_rms_before=0.594 worst_quadrant_rms_after=0.507
verification OK: wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits
verification OK: wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits
Image size: 941.4'x624.4' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 04:36:57.758 +21:57:02.01 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 2454 stars ###
'wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/correct_sextractor_wcs_catalog_usingxy2sky3345006.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 1.703 -> 0.486 arcsec)
WCS_QUALITY_DIAG: file=fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits N_match=1644 sigma_overall_arcsec=0.512 sigma_q1_arcsec=0.518 sigma_q2_arcsec=0.481 sigma_q3_arcsec=0.526 sigma_q4_arcsec=0.562 n_q1=527 n_q2=368 n_q3=513 n_q4=236 worst_quadrant_to_overall_ratio=1.097
The image catalog is written to wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits -region wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_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
############ /tmp/tmp.I8FqkcjDxY (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_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_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_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits
WCS_IMAGE_NAME=wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits
WCS-calibrated image found: wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits
Checking if the catalog wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits.wcscat corresponding to the image wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits.wcscat corresponding to the image wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_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-03-Q2b1x1_2026-07-28_04-18-31_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_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits
WCS catalog name: wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_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=245, bad_region=584, passed=2481
Got 2481 stars (including 1685 good ones) from the SExtractor catalog wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits.wcscat
util/solve_plate_with_UCAC5 got 2481 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.8'
Seting catalog search parameters based on the expected field of view 940.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013067 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010453 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.2)
Done reading UCAC5 zone files...
Matched 1649 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1646 matched stars entering correct_measured_positions(), 1644 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1646 matched stars entering correct_measured_positions(), 1998 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
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 532 to 588 (Dec 16.5 to 27.2)
Done reading UCAC5 zone files...
Matched 1649 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1646 matched stars entering correct_measured_positions(), 1998 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 1646 matched stars entering correct_measured_positions(), 1998 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 1646 stars left (next iteration limit 1810)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=1646 robust_rms=6.300 arcsec worst_quadrant_rms=7.410 arcsec
SIP_REFIT: SIP order 3 trial: matched=1646 robust_rms=0.526 arcsec worst_quadrant_rms=0.545 arcsec
SIP_REFIT: SIP order 5 trial: matched=1646 robust_rms=0.454 arcsec worst_quadrant_rms=0.480 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=1646 robust_rms_before=1.672 arcsec robust_rms_before_corrected=0.498 arcsec robust_rms_after=0.454 arcsec worst_quadrant_rms_before=0.526 worst_quadrant_rms_after=0.480
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.526 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits N_match=1646 sigma_overall_arcsec=0.518 sigma_q1_arcsec=0.515 sigma_q2_arcsec=0.454 sigma_q3_arcsec=0.565 sigma_q4_arcsec=0.544 n_q1=518 n_q2=382 n_q3=508 n_q4=238 worst_quadrant_to_overall_ratio=1.091
The image catalog is written to wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits -region wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_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
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits sigma_overall=0.312 worst_q_ratio=1.271
ref2=Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits sigma_overall=0.303 worst_q_ratio=1.338
new1=fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits sigma_overall=0.512 worst_q_ratio=1.097
new2=fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits sigma_overall=0.518 worst_q_ratio=1.091
reference average sigma_overall=0.3075 worst_q_ratio=1.3045
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161_astrometric_residuals.png (4820 matched stars from wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.28 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162_astrometric_residuals.png (4816 matched stars from wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434_astrometric_residuals.png (1644 matched stars from wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.41 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435_astrometric_residuals.png (1646 matched stars from wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.46 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits'
Saving fully-calibrated image wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits'
Preparing the HTML report for the field Tau-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20616_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435
The candidate 20616_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435 did not pass the final checks
**** FOUND 04:23:57.85 +24:18:14.2 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Tau-03-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-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits
SExtractor catalog cache: saved Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.cat to cache
SExtractor catalog cache: saved Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.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-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_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-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Creating symlink local_wcs_cache/wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits
Creating symlink local_wcs_cache/exclusion_list.txt
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-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits exists and is non-empty
wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits exists and is non-empty
wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits exists and is non-empty
wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits (1st reference image)
verification OK: wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Image size: 941.4'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 04:36:56.001 +21:59:37.88 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-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits (1st new image)
verification OK: wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits
Image size: 940.9'x624.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 04:36:57.621 +21:57:03.66 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 04:36:56.001 +21:59:37.88
Second-epoch image center 04:36:57.621 +21:57:03.66
Angular distance between the image centers 0.0433 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits (2nd new image)
verification OK: wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits
Image size: 940.8'x624.4' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 04:36:55.689 +21:57:37.14 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 04:36:56.001 +21:59:37.88
Second-epoch image center 04:36:55.689 +21:57:37.14
Angular distance between the image centers 0.0336 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 04:36:57.621 +21:57:03.66
Second-epoch second image center 04:36:55.689 +21:57:37.14
Angular distance between the image centers 0.01193 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-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits &> /tmp/tmp.vWE9mRKa7U
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits &> /tmp/tmp.25lOCPUIDC
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits &> /tmp/tmp.eatKf3CuQV
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits &> /tmp/tmp.ipo8lrgALF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits and wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits and wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat
Found non-empty wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits and wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat
The reference image (wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits) and catalog (wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat) found
'wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat' -> 'wcsmag.cat'
Read 86341 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 60.5077 to 78.1095 deg, Dec +16.4682 to +27.2856 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 60.5077 to 78.1095 deg, Dec 16.4682 to 27.2856 deg
Loaded 5191 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): 3474 out of 4349 total matches.
Matched with Tycho-2 4349 out of 86341 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.845350
a=0.000000 b=1.000000 c=22.845350
From vast_summary.log: estimated ref. image limiting mag.: -7.17
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.68
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.68
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 86341 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 60.5077 to 78.1095 deg, Dec +16.4682 to +27.2856 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 60.5077 to 78.1095 deg, Dec 16.4682 to 27.2856 deg
Loaded 5191 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): 3474 out of 4349 total matches.
Matched with Tycho-2 4349 out of 86341 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits:
Forced-photometry filter: calibrated wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits -> calib.txt_param_ref_wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits (aperture=4.4)
Read 85691 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 60.5078 to 78.1091 deg, Dec +16.4883 to +27.2975 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 60.5078 to 78.1091 deg, Dec 16.4883 to 27.2975 deg
Loaded 5188 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): 3464 out of 4347 total matches.
Matched with Tycho-2 4347 out of 85691 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits:
Forced-photometry filter: calibrated wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits -> calib.txt_param_ref_wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits (aperture=4.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 14 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
1.9 pix Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
2.3 pix fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits
2.2 pix fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits
1.9 pix wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
1.9 pix wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
Limiting magnitude estimates:
15.7 mag. Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
15.7 mag. Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
13.5 mag. fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits
13.6 mag. fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits
All-image limiting magnitude estimate: 13.5 (SNR ) 13.2 (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.vWE9mRKa7U (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-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits' -> 'wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
WCS_IMAGE_NAME=wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
WCS-calibrated image found: wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Checking if the catalog wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat corresponding to the image wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits alredy exist and is non-empty...
Catalog wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat corresponding to the image wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
WCS catalog name: wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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=17, blended=6242, bad_region=13891, passed=86324
Got 86324 stars (including 66886 good ones) from the SExtractor catalog wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat
util/solve_plate_with_UCAC5 got 86324 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4862 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4848 matched stars entering correct_measured_positions(), 4848 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4848 matched stars entering correct_measured_positions(), 75480 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4861 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4848 matched stars entering correct_measured_positions(), 75480 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4848 matched stars entering correct_measured_positions(), 75480 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4848 stars left (next iteration limit 5332)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits N_match=4848 sigma_overall_arcsec=0.319 sigma_q1_arcsec=0.396 sigma_q2_arcsec=0.307 sigma_q3_arcsec=0.281 sigma_q4_arcsec=0.252 n_q1=1602 n_q2=612 n_q3=1848 n_q4=786 worst_quadrant_to_overall_ratio=1.241
The image catalog is written to wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits -region wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.25lOCPUIDC (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-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.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_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.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-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.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-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits' -> 'wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.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-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
WCS_IMAGE_NAME=wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
WCS-calibrated image found: wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
Checking if the catalog wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits.wcscat corresponding to the image wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits alredy exist and is non-empty...
Catalog wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits.wcscat corresponding to the image wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
WCS catalog name: wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.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=19, blended=6215, bad_region=13720, passed=85672
Got 85672 stars (including 66440 good ones) from the SExtractor catalog wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits.wcscat
util/solve_plate_with_UCAC5 got 85672 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4864 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4849 matched stars entering correct_measured_positions(), 4850 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4849 matched stars entering correct_measured_positions(), 74972 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4864 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4849 matched stars entering correct_measured_positions(), 74972 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4849 matched stars entering correct_measured_positions(), 74972 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4849 stars left (next iteration limit 5333)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits N_match=4849 sigma_overall_arcsec=0.296 sigma_q1_arcsec=0.386 sigma_q2_arcsec=0.297 sigma_q3_arcsec=0.261 sigma_q4_arcsec=0.229 n_q1=1596 n_q2=617 n_q3=1840 n_q4=796 worst_quadrant_to_overall_ratio=1.305
The image catalog is written to wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits -region wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.eatKf3CuQV (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_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_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_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits
WCS_IMAGE_NAME=wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits
WCS-calibrated image found: wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits
Checking if the catalog wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits.wcscat corresponding to the image wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits.wcscat corresponding to the image wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_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-03-Q2b1x1_2026-07-28_04-17-34_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_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits
WCS catalog name: wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_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=3, blended=563, bad_region=3215, passed=18393
Got 18393 stars (including 14721 good ones) from the SExtractor catalog wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits.wcscat
util/solve_plate_with_UCAC5 got 18393 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.9'
Seting catalog search parameters based on the expected field of view 940.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013068 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010454 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.4 to 27.2)
Done reading UCAC5 zone files...
Matched 4881 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 4864 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 16001 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
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 532 to 588 (Dec 16.4 to 27.2)
Done reading UCAC5 zone files...
Matched 4882 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4866 matched stars entering correct_measured_positions(), 16001 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 4866 matched stars entering correct_measured_positions(), 16001 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 4866 stars left (next iteration limit 5350)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits N_match=4866 sigma_overall_arcsec=0.551 sigma_q1_arcsec=0.547 sigma_q2_arcsec=0.525 sigma_q3_arcsec=0.580 sigma_q4_arcsec=0.564 n_q1=1546 n_q2=970 n_q3=1551 n_q4=799 worst_quadrant_to_overall_ratio=1.052
The image catalog is written to wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits -region wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_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
############ /tmp/tmp.ipo8lrgALF (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_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_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_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits
WCS_IMAGE_NAME=wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits
WCS-calibrated image found: wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits
Checking if the catalog wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits.wcscat corresponding to the image wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits.wcscat corresponding to the image wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_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-03-Q2b1x1_2026-07-28_04-18-31_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_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits
WCS catalog name: wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_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=4, blended=569, bad_region=3329, passed=18717
Got 18717 stars (including 14926 good ones) from the SExtractor catalog wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits.wcscat
util/solve_plate_with_UCAC5 got 18717 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.8'
Seting catalog search parameters based on the expected field of view 940.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013067 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010453 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.2)
Done reading UCAC5 zone files...
Matched 4883 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 4864 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4864 matched stars entering correct_measured_positions(), 16250 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
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 532 to 588 (Dec 16.5 to 27.2)
Done reading UCAC5 zone files...
Matched 4884 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4867 matched stars entering correct_measured_positions(), 16250 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Accuracy estimation diagnostic: 4867 matched stars entering correct_measured_positions(), 16250 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 4867 stars left (next iteration limit 5350)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits N_match=4867 sigma_overall_arcsec=0.527 sigma_q1_arcsec=0.511 sigma_q2_arcsec=0.513 sigma_q3_arcsec=0.553 sigma_q4_arcsec=0.579 n_q1=1549 n_q2=973 n_q3=1539 n_q4=806 worst_quadrant_to_overall_ratio=1.099
The image catalog is written to wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits -region wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_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
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-03-Q2b1x1_2026-07-28_04-17-34_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_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-17-34_20.00sec_-0.00C_LIGHT_0434.fits
Saving fully-calibrated image wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_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_2026-07-28_CI_Tau-03-Q2b1x1_061203_TTUQ2b1x1_2696915_5hDB38LP/wcs_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435.fits
Preparing the HTML report for the field Tau-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:39:30.61 +21:51:21.2: 16.40 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:44:21.54 +22:50:07.3: 13.08 +/- 0.02 detection
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits at 04:39:30.61 +21:51:21.2: 16.37 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits at 04:44:21.54 +22:50:07.3: 13.11 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.10 +/- 0.01
Forced photometry filter KEPT candidate at 04:44:21.54 +22:50:07.3: ref_mag=13.10 +/- 0.01 new_mean_mag=12.1226 delta=0.97 (need > 0.90)
Adding exclusion_list_local.txt__out105629.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35380.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 102333_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435
The candidate 102333_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435 did not pass the final checks
**** FOUND 04:23:57.92 +24:18:14.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 103030_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435
The candidate 103030_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435 did not pass the final checks
**** FOUND 04:28:23.72 +19:10:45.7 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 103799_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435
The candidate 103799_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435 did not pass the final checks
**** FOUND 04:21:45.26 +19:28:43.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 104321_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435
The candidate 104321_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435 did not pass the final checks
**** FOUND 04:42:09.67 +22:55:09.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 104385_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435
The candidate 104385_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435 did not pass the final checks
**** FOUND 04:26:29.18 +22:48:44.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 104576_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435
The candidate 104576_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435 did not pass the final checks
**** FOUND 04:32:07.72 +21:36:44.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 104835_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435
The candidate 104835_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435 did not pass the final checks
**** FOUND 04:48:48.92 +21:18:40.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 104938_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435
The candidate 104938_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435 did not pass the final checks
**** FOUND 04:34:38.45 +22:42:10.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105112_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435
The candidate 105112_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435 did not pass the final checks
**** FOUND 04:26:10.66 +22:49:27.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 105364_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435
The candidate 105364_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435 did not pass the final checks
**** FOUND 04:27:18.08 +23:01:29.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 105540_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435
The candidate 105540_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435 did not pass the final checks
**** FOUND 04:21:32.81 +21:00:55.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105629_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435
Preparing report for the candidate 105629_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435
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Considering the candidate 36988_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435
The candidate 36988_fd_Tau-03-Q2b1x1_2026-07-28_04-18-31_20.00sec_-0.00C_LIGHT_0435 did not pass the final checks