This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
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!
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,2461143.6643,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260413.1643 11.21CV 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 04 13.1643* 05 40 25.95 +21 20 58.4 11.7 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,2461143.6643,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260413.1643 11.71CV 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461082.62137122 11.02.2026 02:54:36.473 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
First image: 2461082.62137122 11.02.2026 02:54:36.473 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
Last image: 2461143.66467889 13.04.2026 03:56:58.256 /data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.68
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 21810
Objects passed selection criteria: 21622
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: 12446.5
Average stars matched: 12011.8 (96.5071 %)
Memory usage VmPeak: 126148 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Apr 12 23:01:39 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461082.62137122 11.02.2026 02:54:36.473 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
First image: 2461082.62137122 11.02.2026 02:54:36.473 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
Last image: 2461143.66467889 13.04.2026 03:56:58.256 /data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 44
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.34
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: 21 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 148788
Objects passed selection criteria: 148248
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: 89165.5
Average stars matched: 85235.2 (95.5922 %)
Memory usage VmPeak: 2091104 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Apr 12 23:05:13 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits
SExtractor catalog cache: saved Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat to cache
SExtractor catalog cache: saved Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.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-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461143.66385375
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-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits exists and is non-empty
Saving wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits to local_wcs_cache/
'wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits' -> 'local_wcs_cache/wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits'
wcs_Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits exists and is non-empty
Saving wcs_Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits to local_wcs_cache/
'wcs_Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits' -> 'local_wcs_cache/wcs_Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits'
wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits exists and is non-empty
Saving wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits to local_wcs_cache/
'wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits' -> 'local_wcs_cache/wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits'
wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits exists and is non-empty
Saving wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits to local_wcs_cache/
'wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits' -> 'local_wcs_cache/wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:32:19.616 +22:00:01.42
Second-epoch image center 05:32:01.110 +22:01:11.16
Angular distance between the image centers 0.0741 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:32:19.616 +22:00:01.42
Second-epoch image center 05:31:58.573 +22:00:43.35
Angular distance between the image centers 0.0821 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 05:32:01.110 +22:01:11.16
Second-epoch second image center 05:31:58.573 +22:00:43.35
Angular distance between the image centers 0.01248 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits &> /tmp/tmp.kfXzKVNQPp
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits &> /tmp/tmp.FHi0jvejhH
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits &> /tmp/tmp.LoD0msX5jC
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits &> /tmp/tmp.oe3nqjsGOv
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.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-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits and wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat
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-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits and wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat
Found non-empty wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits and wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat
The reference image (wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits) and catalog (wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat) found
'wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat' -> 'wcsmag.cat'
Read 23525 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 74.1682 to 91.6910 deg, Dec +16.3328 to +27.3474 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 74.1682 to 91.6910 deg, Dec 16.3328 to 27.3474 deg
Loaded 12326 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): 9058 out of 10254 total matches.
Matched with Tycho-2 10254 out of 23525 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.951925
a=0.000000 b=1.000000 c=22.951925
From vast_summary.log: estimated ref. image limiting mag.: -7.68
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.27
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.27
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
2.3 pix Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
2.5 pix fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits
2.5 pix fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits
Limiting magnitude estimates:
15.3 mag. Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
15.3 mag. Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
11.5 mag. fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits
11.3 mag. fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits
All-image limiting magnitude estimate: 11.3 (SNR ) 9.5 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.kfXzKVNQPp (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.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-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits' -> 'wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
WCS_IMAGE_NAME=wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
WCS-calibrated image found: wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
Checking if the catalog wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat corresponding to the image wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits alredy exist and is non-empty...
Catalog wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat corresponding to the image wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
WCS catalog name: wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2582, passed=23525
Got 23525 stars (including 20915 good ones) from the SExtractor catalog wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat
util/solve_plate_with_UCAC5 got 23525 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
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 898 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 22079 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 22076 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 22076 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 927 stars left (next iteration limit 1020)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits -region wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.FHi0jvejhH (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.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-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits' -> 'wcs_Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
WCS_IMAGE_NAME=wcs_Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
WCS-calibrated image found: wcs_Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
Checking if the catalog wcs_Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat corresponding to the image wcs_Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits alredy exist and is non-empty...
Catalog wcs_Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat corresponding to the image wcs_Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
WCS catalog name: wcs_Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2595, passed=23514
Got 23514 stars (including 20891 good ones) from the SExtractor catalog wcs_Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat
util/solve_plate_with_UCAC5 got 23514 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
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 900 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 22179 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 22181 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 22181 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 926 stars left (next iteration limit 1019)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits -region wcs_Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.LoD0msX5jC (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_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.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_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits
WCS_IMAGE_NAME=wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits
WCS-calibrated image found: wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits
Checking if the catalog wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits.cat corresponding to the image wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits.cat corresponding to the image wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits
WCS catalog name: wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=53, passed=1477
Got 1477 stars (including 1424 good ones) from the SExtractor catalog wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits.cat
util/solve_plate_with_UCAC5 got 1477 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.1 to 27.5)
Done reading UCAC5 zone files...
Matched 914 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 907 matched stars entering correct_measured_positions(), 863 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 907 matched stars entering correct_measured_positions(), 1408 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.1 to 27.5)
Done reading UCAC5 zone files...
Matched 913 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 907 matched stars entering correct_measured_positions(), 1405 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 907 matched stars entering correct_measured_positions(), 1404 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 907 stars left (next iteration limit 997)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits -region wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.oe3nqjsGOv (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_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.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_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits
WCS_IMAGE_NAME=wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits
WCS-calibrated image found: wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits
Checking if the catalog wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits.cat corresponding to the image wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits.cat corresponding to the image wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits
WCS catalog name: wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=52, passed=1586
Got 1586 stars (including 1528 good ones) from the SExtractor catalog wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits.cat
util/solve_plate_with_UCAC5 got 1586 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.1 to 27.4)
Done reading UCAC5 zone files...
Matched 922 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 916 matched stars entering correct_measured_positions(), 872 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 916 matched stars entering correct_measured_positions(), 1510 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
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.1 to 27.4)
Done reading UCAC5 zone files...
Matched 922 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 914 matched stars entering correct_measured_positions(), 1508 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 914 matched stars entering correct_measured_positions(), 1505 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 914 stars left (next iteration limit 1007)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits -region wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits'
Saving fully-calibrated image wcs_Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/wcs_Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits'
Saving fully-calibrated image wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits'
Saving fully-calibrated image wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits'
Preparing the HTML report for the field Tau-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Tau-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits
SExtractor catalog cache: saved Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat to cache
SExtractor catalog cache: saved Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.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-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
Creating symlink local_wcs_cache/wcs_Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits exists and is non-empty
wcs_Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits exists and is non-empty
wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits exists and is non-empty
wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:32:19.616 +22:00:01.42
Second-epoch image center 05:32:01.110 +22:01:11.16
Angular distance between the image centers 0.0741 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:32:19.616 +22:00:01.42
Second-epoch image center 05:31:58.573 +22:00:43.35
Angular distance between the image centers 0.0821 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 05:32:01.110 +22:01:11.16
Second-epoch second image center 05:31:58.573 +22:00:43.35
Angular distance between the image centers 0.01248 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits &> /tmp/tmp.nlNzUF2IUe
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits &> /tmp/tmp.TsIq1cCBDC
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits &> /tmp/tmp.CE6McnRqtg
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits &> /tmp/tmp.PrbBCouQv3
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.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-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits and wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat
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-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits and wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat
Found non-empty wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits and wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat
The reference image (wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits) and catalog (wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat) found
'wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat' -> 'wcsmag.cat'
Read 163644 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 74.1103 to 91.6919 deg, Dec +16.3196 to +27.3524 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 74.1103 to 91.6919 deg, Dec 16.3196 to 27.3524 deg
Loaded 12375 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): 7170 out of 10499 total matches.
Matched with Tycho-2 10499 out of 163644 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.782270
a=0.000000 b=1.000000 c=22.782270
From vast_summary.log: estimated ref. image limiting mag.: -7.34
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.44
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.44
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 44 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
2.0 pix Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
2.3 pix fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits
2.3 pix fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits
Limiting magnitude estimates:
15.4 mag. Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
15.4 mag. Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
12.1 mag. fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits
12.1 mag. fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits
All-image limiting magnitude estimate: 12.1 (SNR ) 11.7 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.nlNzUF2IUe (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.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-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits' -> 'wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
WCS_IMAGE_NAME=wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
WCS-calibrated image found: wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
Checking if the catalog wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat corresponding to the image wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits alredy exist and is non-empty...
Catalog wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat corresponding to the image wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
WCS catalog name: wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=64, blended=21410, passed=163580
Got 163580 stars (including 141899 good ones) from the SExtractor catalog wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat
util/solve_plate_with_UCAC5 got 163580 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
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 904 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 154358 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 154356 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 933 matched stars entering correct_measured_positions(), 154353 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 933 stars left (next iteration limit 1026)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits -region wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.TsIq1cCBDC (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.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-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits' -> 'wcs_Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
WCS_IMAGE_NAME=wcs_Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
WCS-calibrated image found: wcs_Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
Checking if the catalog wcs_Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat corresponding to the image wcs_Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits alredy exist and is non-empty...
Catalog wcs_Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat corresponding to the image wcs_Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
WCS catalog name: wcs_Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=58, blended=21418, passed=163768
Got 163768 stars (including 142082 good ones) from the SExtractor catalog wcs_Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat
util/solve_plate_with_UCAC5 got 163768 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
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 903 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 154424 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 154424 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 154424 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 929 stars left (next iteration limit 1023)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits -region wcs_Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.CE6McnRqtg (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_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.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_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits
WCS_IMAGE_NAME=wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits
WCS-calibrated image found: wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits
Checking if the catalog wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits.cat corresponding to the image wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits.cat corresponding to the image wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits
WCS catalog name: wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=342, passed=15136
Got 15136 stars (including 14760 good ones) from the SExtractor catalog wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits.cat
util/solve_plate_with_UCAC5 got 15136 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.1 to 27.6)
Done reading UCAC5 zone files...
Matched 910 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 903 matched stars entering correct_measured_positions(), 865 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 903 matched stars entering correct_measured_positions(), 14463 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.1 to 27.6)
Done reading UCAC5 zone files...
Matched 910 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 903 matched stars entering correct_measured_positions(), 14464 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 903 matched stars entering correct_measured_positions(), 14447 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 903 stars left (next iteration limit 993)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits -region wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.PrbBCouQv3 (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_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.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_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits
WCS_IMAGE_NAME=wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits
WCS-calibrated image found: wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits
Checking if the catalog wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits.cat corresponding to the image wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits.cat corresponding to the image wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits
WCS catalog name: wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=386, passed=16288
Got 16288 stars (including 15875 good ones) from the SExtractor catalog wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits.cat
util/solve_plate_with_UCAC5 got 16288 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.1 to 27.6)
Done reading UCAC5 zone files...
Matched 918 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 912 matched stars entering correct_measured_positions(), 868 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 912 matched stars entering correct_measured_positions(), 15683 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
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.1 to 27.6)
Done reading UCAC5 zone files...
Matched 918 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 910 matched stars entering correct_measured_positions(), 15684 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 910 matched stars entering correct_measured_positions(), 15671 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 910 stars left (next iteration limit 1003)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits -region wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.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_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/wcs_Tau-04-Q1b1x1_2026-02-10_20-54-36_20.00sec_-15.00C_LIGHT_0038.fits
Saving fully-calibrated image wcs_Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.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_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/wcs_Tau-04-Q1b1x1_2026-02-10_20-55-19_20.00sec_-15.00C_LIGHT_0039.fits
Saving fully-calibrated image wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.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_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-55-46_20.00sec_-4.90C_LIGHTs_0006.fits
Saving fully-calibrated image wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.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_2026-04-12_CI_Tau-04-Q1b1x1_225901_TTUQ1b1x1_2458_jqaoHlJi/wcs_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007.fits
Preparing the HTML report for the field Tau-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out188381.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out188383.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out188387.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out188388.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out189109.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out188732.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189062.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
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
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Considering the candidate 188381_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007
The candidate 188381_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007 did not pass the final checks
**** FOUND 05:58:13.07 +21:57:48.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.67, MAG_FAINT_SEARCH_LIMIT=12.65)GAIADR2_OUTPUT=# 1.448 3424057402795349760 089.55406578290 +21.96358790574 11.9516 11.4563 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.448#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 188382_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007
The candidate 188382_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007 did not pass the final checks
**** FOUND 05:22:27.46 +19:14:10.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 188383_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007
The candidate 188383_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007 did not pass the final checks
**** FOUND 06:02:12.56 +24:40:11.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.18, MAG_FAINT_SEARCH_LIMIT=12.16)GAIADR2_OUTPUT=# 0.226 3426480893932607616 090.55226829126 +24.66979867403 12.0306 11.5856 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.226#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 188384_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007
The candidate 188384_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007 did not pass the final checks
**** FOUND 05:54:54.11 +20:11:09.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 188387_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007
The candidate 188387_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007 did not pass the final checks
**** FOUND 05:49:36.04 +21:49:26.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.78, MAG_FAINT_SEARCH_LIMIT=11.76)GAIADR2_OUTPUT=# 1.962 3400199752819760128 087.39974389084 +21.82443358820 10.9489 10.4943 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.962#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 188388_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007
The candidate 188388_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007 did not pass the final checks
**** FOUND 06:01:10.43 +23:20:05.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.78, MAG_FAINT_SEARCH_LIMIT=11.76)GAIADR2_OUTPUT=# 2.335 3424656499193509248 090.29413785434 +23.33512168767 9.8258 8.4803 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.335#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 188480_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007
The candidate 188480_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007 did not pass the final checks
**** FOUND 04:59:09.36 +19:44:45.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 188619_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007
The candidate 188619_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007 did not pass the final checks
**** FOUND 05:09:42.93 +23:02:02.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 188732_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007
Preparing report for the candidate 188732_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007
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Considering the candidate 189062_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007
Preparing report for the candidate 189062_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007
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Considering the candidate 189109_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007
The candidate 189109_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007 did not pass the final checks
**** FOUND 05:39:10.59 +23:20:17.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 1.742 3404384386697670144 084.79369938394 +23.33836878206 12.0201 11.4302 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.742#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 189112_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007
The candidate 189112_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007 did not pass the final checks
**** FOUND 05:41:56.10 +22:38:55.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 19791_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007
The candidate 19791_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007 did not pass the final checks
**** FOUND 05:01:02.72 +17:30:38.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 162539_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007
The candidate 162539_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007 did not pass the final checks
**** FOUND 05:39:30.48 +26:22:26.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 18025_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007
The candidate 18025_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007 did not pass the final checks
**** FOUND 05:46:56.47 +17:54:30.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 161140_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007
The candidate 161140_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007 did not pass the final checks
**** FOUND 05:09:07.54 +26:08:17.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55654_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007
The candidate 55654_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007 did not pass the final checks
**** FOUND 05:55:48.89 +20:10:31.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 84179_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007
The candidate 84179_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007 did not pass the final checks
**** FOUND 05:27:38.08 +21:56:13.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 70439_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007
The candidate 70439_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007 did not pass the final checks
**** FOUND 05:37:38.53 +21:08:35.1 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 147296_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007
The candidate 147296_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007 did not pass the final checks
**** FOUND 05:35:27.13 +24:02:21.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 88472_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007
The candidate 88472_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007 did not pass the final checks
**** FOUND 05:19:16.82 +22:05:45.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 129173_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007
The candidate 129173_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007 did not pass the final checks
**** FOUND 05:29:16.50 +25:08:58.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 92795_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007
The candidate 92795_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007 did not pass the final checks
**** FOUND 05:15:27.69 +22:17:05.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 29037_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007
The candidate 29037_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007 did not pass the final checks
**** FOUND 05:32:12.80 +18:35:41.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 31463_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007
The candidate 31463_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007 did not pass the final checks
**** FOUND 05:33:31.66 +18:32:26.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 22263_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007
The candidate 22263_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007 did not pass the final checks
**** FOUND 05:27:10.15 +17:57:44.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 119084_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007
The candidate 119084_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007 did not pass the final checks
**** FOUND 05:39:44.22 +25:53:48.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 139525_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007
The candidate 139525_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007 did not pass the final checks
**** FOUND 05:49:00.83 +24:34:02.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 09071_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007
The candidate 09071_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007 did not pass the final checks
**** FOUND 05:28:01.70 +17:14:20.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 13340_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007
The candidate 13340_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007 did not pass the final checks
**** FOUND 05:24:25.96 +17:23:01.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 05938_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007
The candidate 05938_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007 did not pass the final checks
**** FOUND 05:32:14.32 +17:03:26.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 06346_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007
The candidate 06346_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007 did not pass the final checks
**** FOUND 05:37:03.84 +17:02:25.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 144648_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007
The candidate 144648_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007 did not pass the final checks
**** FOUND 05:56:56.12 +24:14:59.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 48649_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007
The candidate 48649_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007 did not pass the final checks
**** FOUND 05:54:56.70 +19:44:59.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 50620_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007
The candidate 50620_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007 did not pass the final checks
**** FOUND 05:52:23.38 +19:52:04.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 37680_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007
The candidate 37680_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007 did not pass the final checks
**** FOUND 05:07:28.04 +18:38:43.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 139224_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007
The candidate 139224_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007 did not pass the final checks
**** FOUND 05:08:06.69 +24:15:54.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 100674_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007
The candidate 100674_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007 did not pass the final checks
**** FOUND 06:04:06.94 +23:15:46.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 55324_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007
The candidate 55324_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007 did not pass the final checks
**** FOUND 06:03:55.10 +20:08:19.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 57459_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007
The candidate 57459_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007 did not pass the final checks
**** FOUND 05:54:22.43 +20:16:34.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 85206_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007
The candidate 85206_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007 did not pass the final checks
**** FOUND 05:03:06.06 +21:35:24.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 15451_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007
The candidate 15451_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007 did not pass the final checks
**** FOUND 05:47:26.19 +17:43:45.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 47689_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007
The candidate 47689_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007 did not pass the final checks
**** FOUND 06:03:27.38 +19:41:26.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 118312_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007
The candidate 118312_fd_Tau-04-Q1b1x1_2026-04-12_22-56-58_20.00sec_-4.90C_LIGHTs_0007 did not pass the final checks