This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7
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 10 22.1908 2461335.6908 10.71 05:22:11.23 +22:53:19.6
182.25206 -7.69714 galactic Tau Second-epoch detections are separated by 0.2" and 2.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.230 Athamantis 1 1 1 11.1 0 0
Forced photometry on wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits at 05:22:11.23 +22:53:19.6: 16.09 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits at 05:22:11.23 +22:53:19.6: 16.00 +/- 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 10 22.1908* 05 22 11.23 +22 53 19.6 10.7 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461335.6908,10.71,0.05,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 20261022.1908 10.71CV 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
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 10 22.1908* 05 21 07.65 +23 38 19.8 12.2 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
V1452 Tau,2461335.6908,12.16,0.05,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
V1452 Tau 20261022.1908 12.16CV 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 10 22.1908 2461335.6908 12.47 05:18:47.96 +20:13:38.1
184.04503 -9.83357 galactic Tau Second-epoch detections are separated by 0.5" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.714 Ulula 0 0 0 13.1 -0 0
Forced photometry on wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits at 05:18:47.96 +20:13:38.1: 16.06 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits at 05:18:47.96 +20:13:38.1: 16.04 +/- 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 10 22.1908* 05 18 47.96 +20 13 38.1 12.5 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,2461335.6908,12.47,0.05,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 20261022.1908 12.47CV 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: 2461032.81064075 23.12.2025 07:27:09.361 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
First image: 2461032.81064075 23.12.2025 07:27:09.361 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Last image: 2461335.69099601 22.10.2026 04:34:52.055 /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.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.: -7.40
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 17391
Objects passed selection criteria: 17233
Measurements per detected object (mean, median, min, max): 2.1 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.1 2.0 2 4
Average stars detected per image: 9927.25
Average stars matched: 9629.25 (96.9982 %)
Memory usage VmPeak: 243576 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Oct 15 15:05:03 CDT 2026
VaST build number 1.0rc89-241-g3eca6a38
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-15)
GNU bash, version 5.3.20(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Oct 21 23:37:28 CDT 2026
Host name: tau
############################################################
ERROR: large change in astrometric-star counts between the two new images (q4: 155 -> 212, 26.887% > 20%; fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits vs fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.81064075 23.12.2025 07:27:09.361 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
First image: 2461032.81064075 23.12.2025 07:27:09.361 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Last image: 2461335.69099601 22.10.2026 04:34:52.055 /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 33
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.07
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: 20 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 132651
Objects passed selection criteria: 132149
Measurements per detected object (mean, median, min, max): 2.2 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.2 2.0 2 4
Average stars detected per image: 78930.2
Average stars matched: 74756.5 (94.7121 %)
Memory usage VmPeak: 603856 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Oct 15 15:05:03 CDT 2026
VaST build number 1.0rc89-241-g3eca6a38
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-15)
GNU bash, version 5.3.20(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Oct 21 23:38:46 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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits
SExtractor catalog cache: saved Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat to cache
SExtractor catalog cache: saved Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits
Checking WCS cache directory local_wcs_cache
Checking 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: 2461335.69054546
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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits exists and is non-empty
wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits exists and is non-empty
wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits exists and is non-empty
wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits (1st reference image)
verification OK: wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Image size: 941.6'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:32:19.570 +21:59:57.74 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-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits (1st new image)
verification OK: wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits
Image size: 941.4'x624.6' 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: 05:32:28.319 +21:59:59.28 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:32:19.570 +21:59:57.74
Second-epoch image center 05:32:28.319 +21:59:59.28
Angular distance between the image centers 0.0338 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits (2nd new image)
verification OK: wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits
Image size: 941.3'x624.6' 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: 05:32:28.064 +22:00:10.38 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:32:19.570 +21:59:57.74
Second-epoch image center 05:32:28.064 +22:00:10.38
Angular distance between the image centers 0.0330 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 05:32:28.319 +21:59:59.28
Second-epoch second image center 05:32:28.064 +22:00:10.38
Angular distance between the image centers 0.00324 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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits &> /tmp/tmp.fjPKUZN50B
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits &> /tmp/tmp.ORahrGCYoz
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits &> /tmp/tmp.TirCOBuA3H
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits &> /tmp/tmp.P61p9VTYPj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits and wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits and wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.wcscat
Found non-empty wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits and wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.wcscat
The reference image (wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits) and catalog (wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.wcscat) found
'wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.wcscat' -> 'wcsmag.cat'
Read 22997 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 74.3514 to 91.9479 deg, Dec +16.4790 to +27.2884 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 74.3514 to 91.9479 deg, Dec 16.4790 to 27.2884 deg
Loaded 12406 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): 8976 out of 10160 total matches.
Matched with Tycho-2 10160 out of 22997 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.969200
a=0.000000 b=1.000000 c=22.969200
From vast_summary.log: estimated ref. image limiting mag.: -7.40
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.57
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.57
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 22997 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 74.3514 to 91.9479 deg, Dec +16.4790 to +27.2884 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 74.3514 to 91.9479 deg, Dec 16.4790 to 27.2884 deg
Loaded 12406 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): 8976 out of 10160 total matches.
Matched with Tycho-2 10160 out of 22997 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Forced-photometry filter: calibrated wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits -> calib.txt_param_ref_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits (aperture=6.0)
Read 20916 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 74.3773 to 91.9061 deg, Dec +16.4876 to +27.3008 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 74.3773 to 91.9061 deg, Dec 16.4876 to 27.3008 deg
Loaded 12329 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): 8847 out of 10017 total matches.
Matched with Tycho-2 10017 out of 20916 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
Forced-photometry filter: calibrated wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits -> calib.txt_param_ref_wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
2.0 pix Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
2.7 pix fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits
2.7 pix fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits
Limiting magnitude estimates:
15.6 mag. Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
15.5 mag. Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
13.1 mag. fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits
12.9 mag. fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits
All-image limiting magnitude estimate: 12.9 (SNR ) 10.5 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.fjPKUZN50B (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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits' -> 'wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
WCS_IMAGE_NAME=wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
WCS-calibrated image found: wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Checking if the catalog wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.wcscat corresponding to the image wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits alredy exist and is non-empty...
Catalog wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.wcscat corresponding to the image wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
WCS catalog name: wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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=2479, bad_region=3694, passed=22997
Got 22997 stars (including 17090 good ones) from the SExtractor catalog wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.wcscat
util/solve_plate_with_UCAC5 got 22997 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4775 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4705 matched stars entering correct_measured_positions(), 4706 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4705 matched stars entering correct_measured_positions(), 20056 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
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 4774 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4705 matched stars entering correct_measured_positions(), 20056 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4705 matched stars entering correct_measured_positions(), 20056 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 4705 stars left (next iteration limit 5175)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits N_match=4705 sigma_overall_arcsec=0.386 sigma_q1_arcsec=0.461 sigma_q2_arcsec=0.374 sigma_q3_arcsec=0.350 sigma_q4_arcsec=0.273 n_q1=1788 n_q2=376 n_q3=1844 n_q4=697 worst_quadrant_to_overall_ratio=1.193
WCS_HEADER_DIAG: file=Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits selection=current_pairs N_selected=4705 N_valid=4705 bias_ra_arcsec=0.002 bias_dec_arcsec=-0.009 median_sep_arcsec=0.265 p95_sep_arcsec=1.655 n_q1=1788 n_q2=376 n_q3=1844 n_q4=697 occupied_cells_4x4=16/16
The image catalog is written to wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits -region wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.ORahrGCYoz (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-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.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_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.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-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.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-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits' -> 'wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.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-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
WCS_IMAGE_NAME=wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
WCS-calibrated image found: wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
Checking if the catalog wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits.wcscat corresponding to the image wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits alredy exist and is non-empty...
Catalog wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits.wcscat corresponding to the image wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
WCS catalog name: wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.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=2320, bad_region=3377, passed=20916
Got 20916 stars (including 15475 good ones) from the SExtractor catalog wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits.wcscat
util/solve_plate_with_UCAC5 got 20916 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4776 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4707 matched stars entering correct_measured_positions(), 4708 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4707 matched stars entering correct_measured_positions(), 18215 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
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 4777 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4708 matched stars entering correct_measured_positions(), 18215 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 4708 matched stars entering correct_measured_positions(), 18215 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 4708 stars left (next iteration limit 5177)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits N_match=4708 sigma_overall_arcsec=0.515 sigma_q1_arcsec=0.605 sigma_q2_arcsec=0.498 sigma_q3_arcsec=0.464 sigma_q4_arcsec=0.402 n_q1=1784 n_q2=371 n_q3=1863 n_q4=690 worst_quadrant_to_overall_ratio=1.175
WCS_HEADER_DIAG: file=Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits selection=current_pairs N_selected=4708 N_valid=4708 bias_ra_arcsec=0.005 bias_dec_arcsec=-0.010 median_sep_arcsec=0.365 p95_sep_arcsec=1.905 n_q1=1784 n_q2=371 n_q3=1863 n_q4=690 occupied_cells_4x4=16/16
The image catalog is written to wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits -region wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.TirCOBuA3H (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_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.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_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits
WCS_IMAGE_NAME=wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits
WCS-calibrated image found: wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits
Checking if the catalog wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits.wcscat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits.wcscat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits
WCS catalog name: wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.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=136, bad_region=421, passed=1910
Got 1910 stars (including 1376 good ones) from the SExtractor catalog wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits.wcscat
util/solve_plate_with_UCAC5 got 1910 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 1332 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1318 matched stars entering correct_measured_positions(), 1310 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1318 matched stars entering correct_measured_positions(), 1481 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
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 1331 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1316 matched stars entering correct_measured_positions(), 1481 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.79"
Accuracy estimation diagnostic: 1316 matched stars entering correct_measured_positions(), 1481 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
Excluding outliers - 1316 stars left (next iteration limit 1449)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=1316 robust_rms=6.117 arcsec worst_region_rms=8.315 arcsec outer_annulus_rms=8.159 arcsec
SIP_REFIT: SIP order 3 trial: matched=1316 robust_rms=0.801 arcsec worst_region_rms=0.918 arcsec outer_annulus_rms=0.918 arcsec
SIP_REFIT: SIP order 5 trial: matched=1316 robust_rms=0.642 arcsec worst_region_rms=0.863 arcsec outer_annulus_rms=0.863 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=1316 robust_rms_before=1.697 arcsec robust_rms_before_corrected=0.769 arcsec robust_rms_after=0.642 arcsec worst_region_rms_before=1.040 worst_region_rms_after=0.863 outer_annulus_rms_before=1.760 outer_annulus_rms_after=0.863
verification OK: wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits.sip_refit.sXFq45/candidate.fits
verification OK: wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits.sip_refit.sXFq45/candidate.fits
Image size: 941.2'x624.7' 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: 05:32:28.314 +21:59:58.04 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 1910 stars ###
'wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits.sip_refit.sXFq45/candidate.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction_2801333.cat.log'
'wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits.sip_refit.sXFq45/candidate.wcscat.xy2sky.eoWPVS' -> 'vast_debug_catalog_after_xy2sky_correction_2801333.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 1.697 -> 0.642 arcsec)
SIP_REFIT: re-matching the catalog with the refit solution (cycle 1, search radius 3.2 arcsec, 1316 pairs from the previous matching)
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 1238 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
SIP_REFIT: re-match found 1238 pairs (1316 from the previous matching)
SIP_REFIT: SIP order 2 trial: matched=1238 robust_rms=5.997 arcsec worst_region_rms=8.142 arcsec outer_annulus_rms=7.938 arcsec
SIP_REFIT: SIP order 3 trial: matched=1238 robust_rms=0.791 arcsec worst_region_rms=0.872 arcsec outer_annulus_rms=0.872 arcsec
SIP_REFIT: SIP order 5 trial: matched=1238 robust_rms=0.633 arcsec worst_region_rms=0.867 arcsec outer_annulus_rms=0.867 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=1238 robust_rms_before=0.634 arcsec robust_rms_before_corrected=0.634 arcsec robust_rms_after=0.791 arcsec worst_region_rms_before=0.857 worst_region_rms_after=0.872 outer_annulus_rms_before=0.857 outer_annulus_rms_after=0.872
SIP_REFIT: the refit on the re-matched pairs is worse than the solution it would replace (worst-region 0.872 vs 0.857 arcsec) - keeping the current solution
SIP_REFIT: the refit on the re-matched pairs was not applied - keeping the current solution
Accuracy estimation diagnostic: 1238 matched stars entering correct_measured_positions(), 1478 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Accuracy estimation diagnostic: 1238 matched stars entering correct_measured_positions(), 1476 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
WCS_QUALITY_DIAG: file=fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits N_match=1238 sigma_overall_arcsec=0.640 sigma_q1_arcsec=0.614 sigma_q2_arcsec=0.428 sigma_q3_arcsec=0.756 sigma_q4_arcsec=0.535 n_q1=454 n_q2=90 n_q3=539 n_q4=155 worst_quadrant_to_overall_ratio=1.182
WCS_HEADER_DIAG: file=fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits selection=current_pairs N_selected=1238 N_valid=1238 bias_ra_arcsec=-0.025 bias_dec_arcsec=0.003 median_sep_arcsec=0.510 p95_sep_arcsec=1.482 n_q1=454 n_q2=90 n_q3=539 n_q4=155 occupied_cells_4x4=15/16
The image catalog is written to wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits -region wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.P61p9VTYPj (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_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.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_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits
WCS_IMAGE_NAME=wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits
WCS-calibrated image found: wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits
Checking if the catalog wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits.wcscat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits.wcscat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits
WCS catalog name: wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.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=132, bad_region=413, passed=2040
Got 2040 stars (including 1509 good ones) from the SExtractor catalog wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits.wcscat
util/solve_plate_with_UCAC5 got 2040 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 1453 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1438 matched stars entering correct_measured_positions(), 1430 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1438 matched stars entering correct_measured_positions(), 1616 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
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 1452 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1437 matched stars entering correct_measured_positions(), 1616 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Accuracy estimation diagnostic: 1437 matched stars entering correct_measured_positions(), 1616 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Excluding outliers - 1437 stars left (next iteration limit 1581)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: the 1437 catalog matches do not cover the frame (534/85/606/212 per quadrant, need 89 in each) - keeping the original solution
WCS_QUALITY_DIAG: file=fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits N_match=1437 sigma_overall_arcsec=0.775 sigma_q1_arcsec=0.672 sigma_q2_arcsec=1.021 sigma_q3_arcsec=0.886 sigma_q4_arcsec=0.593 n_q1=534 n_q2=85 n_q3=606 n_q4=212 worst_quadrant_to_overall_ratio=1.318
WCS_HEADER_DIAG: file=fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits selection=current_pairs N_selected=1437 N_valid=1437 bias_ra_arcsec=0.765 bias_dec_arcsec=0.200 median_sep_arcsec=1.364 p95_sep_arcsec=3.793 n_q1=534 n_q2=85 n_q3=606 n_q4=212 occupied_cells_4x4=15/16
The image catalog is written to wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits -region wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits to local_wcs_cache/
'wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits' -> 'local_wcs_cache/wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits'
Saving the final (post-refit) wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits to local_wcs_cache/
'wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits' -> 'local_wcs_cache/wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits'
Saving the final (post-refit) wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits to local_wcs_cache/
'wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits' -> 'local_wcs_cache/wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits'
Saving the final (post-refit) wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits to local_wcs_cache/
'wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits' -> 'local_wcs_cache/wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits sigma_overall=0.386 worst_q_ratio=1.193
ref2=Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits sigma_overall=0.515 worst_q_ratio=1.175
new1=fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits sigma_overall=0.640 worst_q_ratio=1.182
new2=fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits sigma_overall=0.775 worst_q_ratio=1.318
reference average sigma_overall=0.4505 worst_q_ratio=1.184
warn-on-ratio threshold: 2.0x reference
###################################
ERROR: large change in astrometric-star counts between the two new images (q4: 155 -> 212, 26.887% > 20%; fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits vs fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits) - usually a bad plate solution on one of them, sometimes stars crossing a quadrant boundary when the two images are widely offset, rarely a transparency change; continuing processing
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378_astrometric_residuals.png (4705 matched stars from wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035_astrometric_residuals.png (4708 matched stars from wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.47 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187_astrometric_residuals.png (1238 matched stars from wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.46 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188_astrometric_residuals.png (1437 matched stars from wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.65 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits'
Saving fully-calibrated image wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits'
Preparing the HTML report for the field Tau-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits at 05:22:11.23 +22:53:19.6: 16.09 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits at 05:22:11.23 +22:53:19.6: 16.00 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out31093.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31093_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188
Preparing report for the candidate 31093_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 8s
Prepared the HTML report for the field Tau-04-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 ####
05:22:11.23 +22:53:19.6
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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits
SExtractor catalog cache: saved Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.cat to cache
SExtractor catalog cache: saved Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Creating symlink local_wcs_cache/wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits
Checking 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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits exists and is non-empty
wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits exists and is non-empty
wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits exists and is non-empty
wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits (1st reference image)
verification OK: wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Image size: 941.6'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:32:19.570 +21:59:57.74 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-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits (1st new image)
verification OK: wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits
Image size: 941.2'x624.7' 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: 05:32:28.314 +21:59:58.04 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:32:19.570 +21:59:57.74
Second-epoch image center 05:32:28.314 +21:59:58.04
Angular distance between the image centers 0.0338 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits (2nd new image)
verification OK: wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits
Image size: 941.3'x624.6' 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: 05:32:28.064 +22:00:10.38 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:32:19.570 +21:59:57.74
Second-epoch image center 05:32:28.064 +22:00:10.38
Angular distance between the image centers 0.0330 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 05:32:28.314 +21:59:58.04
Second-epoch second image center 05:32:28.064 +22:00:10.38
Angular distance between the image centers 0.00356 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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits &> /tmp/tmp.7rMo29MxHV
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits &> /tmp/tmp.YES6o0ixN8
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits &> /tmp/tmp.nJGZgJS3Ji
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits &> /tmp/tmp.h31ucDaajl
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits and wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits and wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.wcscat
Found non-empty wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits and wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.wcscat
The reference image (wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits) and catalog (wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.wcscat) found
'wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.wcscat' -> 'wcsmag.cat'
Read 167968 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 74.3408 to 91.9478 deg, Dec +16.4791 to +27.2941 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 74.3408 to 91.9478 deg, Dec 16.4791 to 27.2941 deg
Loaded 12414 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): 7145 out of 10502 total matches.
Matched with Tycho-2 10502 out of 167968 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.825500
a=0.000000 b=1.000000 c=22.825500
From vast_summary.log: estimated ref. image limiting mag.: -7.07
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.76
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.76
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 167968 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 74.3408 to 91.9478 deg, Dec +16.4791 to +27.2941 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 74.3408 to 91.9478 deg, Dec 16.4791 to 27.2941 deg
Loaded 12414 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): 7145 out of 10502 total matches.
Matched with Tycho-2 10502 out of 167968 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Forced-photometry filter: calibrated wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits -> calib.txt_param_ref_wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits (aperture=4.5)
Read 163013 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 74.3370 to 91.9475 deg, Dec +16.4845 to +27.3051 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 74.3370 to 91.9475 deg, Dec 16.4845 to 27.3051 deg
Loaded 12419 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): 7184 out of 10475 total matches.
Matched with Tycho-2 10475 out of 163013 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
Forced-photometry filter: calibrated wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits -> calib.txt_param_ref_wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits (aperture=4.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 25 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
1.8 pix Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
2.4 pix fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits
2.4 pix fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits
Limiting magnitude estimates:
15.8 mag. Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
15.7 mag. Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
13.5 mag. fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits
13.5 mag. fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits
All-image limiting magnitude estimate: 13.5 (SNR ) 12.9 (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.7rMo29MxHV (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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits' -> 'wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
WCS_IMAGE_NAME=wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
WCS-calibrated image found: wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
Checking if the catalog wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.wcscat corresponding to the image wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits alredy exist and is non-empty...
Catalog wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.wcscat corresponding to the image wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits
WCS catalog name: wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.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=28, blended=21684, bad_region=23036, passed=167940
Got 167940 stars (including 124901 good ones) from the SExtractor catalog wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.wcscat
util/solve_plate_with_UCAC5 got 167940 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4762 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4714 matched stars entering correct_measured_positions(), 4714 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4714 matched stars entering correct_measured_positions(), 150202 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4763 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4713 matched stars entering correct_measured_positions(), 150202 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4713 matched stars entering correct_measured_positions(), 150201 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 4713 stars left (next iteration limit 5185)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits N_match=4713 sigma_overall_arcsec=0.381 sigma_q1_arcsec=0.470 sigma_q2_arcsec=0.365 sigma_q3_arcsec=0.343 sigma_q4_arcsec=0.295 n_q1=1719 n_q2=436 n_q3=1839 n_q4=719 worst_quadrant_to_overall_ratio=1.232
WCS_HEADER_DIAG: file=Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits selection=current_pairs N_selected=4713 N_valid=4713 bias_ra_arcsec=-0.006 bias_dec_arcsec=-0.002 median_sep_arcsec=0.255 p95_sep_arcsec=1.454 n_q1=1719 n_q2=436 n_q3=1839 n_q4=719 occupied_cells_4x4=16/16
The image catalog is written to wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits -region wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.YES6o0ixN8 (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-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.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_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.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-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.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-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits' -> 'wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.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-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
WCS_IMAGE_NAME=wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
WCS-calibrated image found: wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
Checking if the catalog wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits.wcscat corresponding to the image wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits alredy exist and is non-empty...
Catalog wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits.wcscat corresponding to the image wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits
WCS catalog name: wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.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=36, blended=20219, bad_region=22244, passed=162977
Got 162977 stars (including 121992 good ones) from the SExtractor catalog wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits.wcscat
util/solve_plate_with_UCAC5 got 162977 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4760 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4706 matched stars entering correct_measured_positions(), 4706 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4706 matched stars entering correct_measured_positions(), 145759 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
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 4760 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4705 matched stars entering correct_measured_positions(), 145759 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 4704 matched stars entering correct_measured_positions(), 145759 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 4704 stars left (next iteration limit 5176)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits N_match=4704 sigma_overall_arcsec=0.497 sigma_q1_arcsec=0.615 sigma_q2_arcsec=0.464 sigma_q3_arcsec=0.445 sigma_q4_arcsec=0.412 n_q1=1720 n_q2=418 n_q3=1843 n_q4=723 worst_quadrant_to_overall_ratio=1.238
WCS_HEADER_DIAG: file=Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits selection=current_pairs N_selected=4704 N_valid=4704 bias_ra_arcsec=0.002 bias_dec_arcsec=0.002 median_sep_arcsec=0.347 p95_sep_arcsec=1.639 n_q1=1720 n_q2=418 n_q3=1843 n_q4=723 occupied_cells_4x4=16/16
The image catalog is written to wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits -region wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.nJGZgJS3Ji (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_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.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_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits
WCS_IMAGE_NAME=wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits
WCS-calibrated image found: wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits
Checking if the catalog wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits.wcscat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits.wcscat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits
WCS catalog name: wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=755, bad_region=4240, passed=19720
Got 19720 stars (including 14837 good ones) from the SExtractor catalog wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits.wcscat
util/solve_plate_with_UCAC5 got 19720 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (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 27.3)
Done reading UCAC5 zone files...
Matched 4809 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4749 matched stars entering correct_measured_positions(), 4744 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4748 matched stars entering correct_measured_positions(), 15808 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
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 27.3)
Done reading UCAC5 zone files...
Matched 4810 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4749 matched stars entering correct_measured_positions(), 15809 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Accuracy estimation diagnostic: 4749 matched stars entering correct_measured_positions(), 15809 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
Excluding outliers - 4749 stars left (next iteration limit 5222)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4749 robust_rms=6.276 arcsec worst_region_rms=8.797 arcsec outer_annulus_rms=8.797 arcsec
SIP_REFIT: SIP order 3 trial: matched=4749 robust_rms=0.930 arcsec worst_region_rms=1.128 arcsec outer_annulus_rms=1.128 arcsec
SIP_REFIT: SIP order 5 trial: matched=4749 robust_rms=0.748 arcsec worst_region_rms=1.064 arcsec outer_annulus_rms=1.064 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4749 robust_rms_before=0.752 arcsec robust_rms_before_corrected=0.782 arcsec robust_rms_after=0.748 arcsec worst_region_rms_before=1.126 worst_region_rms_after=1.064 outer_annulus_rms_before=1.126 outer_annulus_rms_after=1.064
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 1.126 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits worst_region_rms_kept=1.126 arcsec robust_rms_kept=0.752 arcsec matched=4749
WCS_QUALITY_DIAG: file=fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits N_match=4749 sigma_overall_arcsec=0.742 sigma_q1_arcsec=0.668 sigma_q2_arcsec=0.560 sigma_q3_arcsec=0.931 sigma_q4_arcsec=0.567 n_q1=1716 n_q2=452 n_q3=1989 n_q4=592 worst_quadrant_to_overall_ratio=1.256
WCS_HEADER_DIAG: file=fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits selection=current_pairs N_selected=4749 N_valid=4749 bias_ra_arcsec=0.031 bias_dec_arcsec=-0.015 median_sep_arcsec=0.600 p95_sep_arcsec=2.629 n_q1=1716 n_q2=452 n_q3=1989 n_q4=592 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits -region wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.h31ucDaajl (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_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.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_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits
WCS_IMAGE_NAME=wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits
WCS-calibrated image found: wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits
Checking if the catalog wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits.wcscat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits.wcscat corresponding to the image wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits
WCS catalog name: wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.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=793, bad_region=3983, passed=20342
Got 20342 stars (including 15686 good ones) from the SExtractor catalog wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits.wcscat
util/solve_plate_with_UCAC5 got 20342 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 16.4 to 27.3)
Done reading UCAC5 zone files...
Matched 4814 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4751 matched stars entering correct_measured_positions(), 4752 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4751 matched stars entering correct_measured_positions(), 16628 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
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 27.3)
Done reading UCAC5 zone files...
Matched 4814 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4749 matched stars entering correct_measured_positions(), 16627 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Accuracy estimation diagnostic: 4749 matched stars entering correct_measured_positions(), 16627 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
Excluding outliers - 4749 stars left (next iteration limit 5226)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4749 robust_rms=6.351 arcsec worst_region_rms=9.762 arcsec outer_annulus_rms=9.762 arcsec
SIP_REFIT: SIP order 3 trial: matched=4749 robust_rms=0.899 arcsec worst_region_rms=1.222 arcsec outer_annulus_rms=1.222 arcsec
SIP_REFIT: SIP order 5 trial: matched=4749 robust_rms=0.729 arcsec worst_region_rms=1.054 arcsec outer_annulus_rms=1.054 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4749 robust_rms_before=1.815 arcsec robust_rms_before_corrected=0.763 arcsec robust_rms_after=0.729 arcsec worst_region_rms_before=1.177 worst_region_rms_after=1.054 outer_annulus_rms_before=2.088 outer_annulus_rms_after=1.054
SIP_REFIT: applied the refit solution to the output catalog positions only (order 5, robust RMS 1.815 -> 0.729 arcsec); the image header was NOT rewritten as wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits is a symbolic link
SIP_REFIT: re-matching the catalog with the refit solution (cycle 1, search radius 3.6 arcsec, 4749 pairs from the previous matching)
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 27.3)
Done reading UCAC5 zone files...
Matched 4566 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
SIP_REFIT: re-match found 4566 pairs (4749 from the previous matching)
SIP_REFIT: wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4566 robust_rms=6.291 arcsec worst_region_rms=9.422 arcsec outer_annulus_rms=9.422 arcsec
SIP_REFIT: SIP order 3 trial: matched=4566 robust_rms=0.888 arcsec worst_region_rms=1.163 arcsec outer_annulus_rms=1.163 arcsec
SIP_REFIT: SIP order 5 trial: matched=4566 robust_rms=0.719 arcsec worst_region_rms=1.006 arcsec outer_annulus_rms=1.006 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4566 robust_rms_before=0.720 arcsec robust_rms_before_corrected=0.720 arcsec robust_rms_after=0.719 arcsec worst_region_rms_before=1.006 worst_region_rms_after=1.006 outer_annulus_rms_before=1.006 outer_annulus_rms_after=1.006
SIP_REFIT: applied the refit solution to the output catalog positions only (order 5, robust RMS 0.720 -> 0.719 arcsec); the image header was NOT rewritten as wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits is a symbolic link
Accuracy estimation diagnostic: 4566 matched stars entering correct_measured_positions(), 16628 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Accuracy estimation diagnostic: 4566 matched stars entering correct_measured_positions(), 16621 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
WCS_QUALITY_DIAG: file=fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits N_match=4566 sigma_overall_arcsec=0.714 sigma_q1_arcsec=0.675 sigma_q2_arcsec=0.628 sigma_q3_arcsec=0.879 sigma_q4_arcsec=0.586 n_q1=1709 n_q2=369 n_q3=1834 n_q4=654 worst_quadrant_to_overall_ratio=1.230
WCS_HEADER_DIAG: file=fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits selection=current_pairs N_selected=4566 N_valid=4566 bias_ra_arcsec=0.854 bias_dec_arcsec=0.236 median_sep_arcsec=1.482 p95_sep_arcsec=3.347 n_q1=1709 n_q2=369 n_q3=1834 n_q4=654 occupied_cells_4x4=16/16
The image catalog is written to wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits -region wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.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_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-13_20.00sec_-0.00C_LIGHT_0187.fits
Saving fully-calibrated image wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.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_2026-10-21_CI_Tau-04-Q2b1x1_233523_TTUQ2b1x1_2773217_FGSCdvj7/wcs_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188.fits
Preparing the HTML report for the field Tau-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits at 05:20:07.88 +20:29:15.8: 12.54 +/- 0.01 detection
Forced photometry on wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits at 05:18:47.96 +20:13:38.1: 16.06 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-04-Q2b1x1_2025-12-23_01-27-09_20.00sec_-15.00C_LIGHT_0378.fits at 05:13:04.91 +20:18:41.5: 99.00 +/- 99.00 bad_region
Forced photometry on wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits at 05:20:07.88 +20:29:15.8: 12.61 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.01
Forced photometry filter REJECTED candidate at 05:20:07.88 +20:29:15.8: ref_mag=12.57 +/- 0.01 new_mean_mag=12.6036 delta=-0.04 (need > 0.90)
Forced photometry on wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits at 05:18:47.96 +20:13:38.1: 16.04 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-04-Q2b1x1_2026-02-21_20-27-39_20.00sec_-14.90C_LIGHT_0035.fits at 05:13:04.91 +20:18:41.5: 13.29 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.03
Forced photometry filter REJECTED candidate at 05:13:04.91 +20:18:41.5: ref_mag=13.29 +/- 0.03 new_mean_mag=13.0715 delta=0.22 (need > 0.90)
Adding exclusion_list_local.txt__out191709.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 12s
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
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189035_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188
The candidate 189035_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188 did not pass the final checks
**** FOUND 05:44:45.64 +17:48:33.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189038_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188
The candidate 189038_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189300_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188
The candidate 189300_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189534_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188
The candidate 189534_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188 did not pass the final checks
**** FOUND 05:22:11.21 +22:53:19.7 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 189866_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188
The candidate 189866_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190413_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188
The candidate 190413_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190702_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188
The candidate 190702_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190786_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188
The candidate 190786_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191026_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188
The candidate 191026_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191044_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188
Preparing report for the candidate 191044_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191381_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188
The candidate 191381_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188 did not pass the final checks
**** FOUND 05:30:50.64 +22:27:24.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191709_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188
Preparing report for the candidate 191709_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191808_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188
The candidate 191808_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188 did not pass the final checks
**** FOUND 05:20:11.76 +19:34:18.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 192663_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188
The candidate 192663_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193148_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188
The candidate 193148_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193162_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188
The candidate 193162_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193332_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188
The candidate 193332_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188 did not pass the final checks
Rejecting candidate due to large distance (12.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193391_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188
The candidate 193391_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193522_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188
The candidate 193522_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 193575_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188
The candidate 193575_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 180001_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188
The candidate 180001_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 80518_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188
The candidate 80518_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116626_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188
The candidate 116626_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133517_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188
The candidate 133517_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18816_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188
The candidate 18816_fd_Tau-04-Q2b1x1_2026-10-21_23-34-52_20.00sec_-0.00C_LIGHT_0188 did not pass the final checks