This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX
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!
TCP 2026 04 08.4499* 08 54 00.75 +65 57 27.2 13.0 U UMa 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461138.9500,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260408.4500 12.96CV 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 08.4499* 08 52 21.00 +66 07 40.1 12.5 U UMa 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1092850648895987840,2461138.9500,12.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1092850648895987840 20260408.4500 12.50CV 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: 2461093.76297353 22.02.2026 06:18:30.913 /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits
First image: 2461093.76297353 22.02.2026 06:18:30.913 /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits
Last image: 2461138.95023698 08.04.2026 10:48:10.475 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.51
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 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): 6609
Objects passed selection criteria: 6589
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 5330.25
Average stars matched: 5162.5 (96.8529 %)
Memory usage VmPeak: 113080 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Apr 8 05:51:09 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461093.76297353 22.02.2026 06:18:30.913 /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits
First image: 2461093.76297353 22.02.2026 06:18:30.913 /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits
Last image: 2461138.95023698 08.04.2026 10:48:10.475 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 34
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.18
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: 12 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): 38214
Objects passed selection criteria: 38102
Measurements per detected object (mean, median, min, max): 3.1 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 3.0 2 4
Average stars detected per image: 30864.2
Average stars matched: 29667.5 (96.1225 %)
Memory usage VmPeak: 143320 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Apr 8 05:51:51 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits
SExtractor catalog cache: saved UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits.cat to cache
SExtractor catalog cache: saved UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.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/UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.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: 2461138.94967256
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_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits exists and is non-empty
Saving wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits to local_wcs_cache/
'wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits' -> 'local_wcs_cache/wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits'
wcs_UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits exists and is non-empty
Saving wcs_UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits to local_wcs_cache/
'wcs_UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits' -> 'local_wcs_cache/wcs_UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits'
wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits exists and is non-empty
Saving wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits to local_wcs_cache/
'wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits' -> 'local_wcs_cache/wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits'
wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits exists and is non-empty
Saving wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits to local_wcs_cache/
'wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits' -> 'local_wcs_cache/wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.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 09:36:12.813 +69:59:27.41
Second-epoch image center 09:36:01.626 +69:55:46.09
Angular distance between the image centers 0.0635 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 09:36:12.813 +69:59:27.41
Second-epoch image center 09:36:03.318 +69:56:15.01
Angular distance between the image centers 0.0551 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 09:36:01.626 +69:55:46.09
Second-epoch second image center 09:36:03.318 +69:56:15.01
Angular distance between the image centers 0.00839 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/UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits &> /tmp/tmp.vY1SRylum9
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits &> /tmp/tmp.oacmDSJJpp
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits &> /tmp/tmp.PIK4Th83eZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits &> /tmp/tmp.9phG928f6Z
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits
Calibrating the magnitude scale
Found non-empty wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.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_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits and wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.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_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits and wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits.cat
Found non-empty wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits and wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits.cat
The reference image (wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits) and catalog (wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits.cat) found
'wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits.cat' -> 'wcsmag.cat'
Read 9450 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 116.6936 to 171.9946 deg, Dec +62.9087 to +75.4796 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 116.6936 to 171.9946 deg, Dec 62.9087 to 75.4796 deg
Loaded 9371 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): 5144 out of 5451 total matches.
Matched with Tycho-2 5451 out of 9450 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.910180
a=0.000000 b=1.000000 c=22.910180
From vast_summary.log: estimated ref. image limiting mag.: -7.51
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.40
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.40
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits
2.2 pix UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits
2.6 pix fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits
2.6 pix fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits
Limiting magnitude estimates:
15.4 mag. UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits
15.4 mag. UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits
14.4 mag. fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits
14.4 mag. fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 11.7 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.vY1SRylum9 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits' -> 'wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits
WCS_IMAGE_NAME=wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits
WCS-calibrated image found: wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits
Checking if the catalog wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits.cat corresponding to the image wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits alredy exist and is non-empty...
Catalog wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits.cat corresponding to the image wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits
WCS catalog name: wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=712, passed=9450
Got 9450 stars (including 8721 good ones) from the SExtractor catalog wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits.cat
util/solve_plate_with_UCAC5 got 9450 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.9 to 75.5)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 957 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 9331 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 764 to 829 (Dec 62.9 to 75.5)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 9330 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
WARNING: Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 9330 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits -region wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.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.oacmDSJJpp (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits' -> 'wcs_UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits
WCS_IMAGE_NAME=wcs_UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits
WCS-calibrated image found: wcs_UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits
Checking if the catalog wcs_UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits.cat corresponding to the image wcs_UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits alredy exist and is non-empty...
Catalog wcs_UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits.cat corresponding to the image wcs_UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits
WCS catalog name: wcs_UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=727, passed=9454
Got 9454 stars (including 8716 good ones) from the SExtractor catalog wcs_UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits.cat
util/solve_plate_with_UCAC5 got 9454 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.9 to 75.5)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 9351 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 764 to 829 (Dec 62.9 to 75.5)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 9351 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
WARNING: Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 9351 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits -region wcs_UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.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.PIK4Th83eZ (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_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.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_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits
WCS_IMAGE_NAME=wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits
WCS-calibrated image found: wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits
Checking if the catalog wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits.cat corresponding to the image wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits.cat corresponding to the image wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits
WCS catalog name: wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=423, passed=5143
Got 5143 stars (including 4720 good ones) from the SExtractor catalog wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits.cat
util/solve_plate_with_UCAC5 got 5143 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 768 to 827 (Dec 63.7 to 75.2)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 5113 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 768 to 827 (Dec 63.7 to 75.2)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 5113 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
WARNING: Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 5113 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits -region wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.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.9phG928f6Z (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_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.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_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits
WCS_IMAGE_NAME=wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits
WCS-calibrated image found: wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits
Checking if the catalog wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits.cat corresponding to the image wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits.cat corresponding to the image wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits
WCS catalog name: wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=455, passed=5171
Got 5171 stars (including 4714 good ones) from the SExtractor catalog wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits.cat
util/solve_plate_with_UCAC5 got 5171 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 768 to 828 (Dec 63.7 to 75.2)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 960 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 5137 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 768 to 828 (Dec 63.7 to 75.2)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 5137 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
WARNING: Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 5137 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits -region wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.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_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits'
Saving fully-calibrated image wcs_UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/wcs_UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits'
Saving fully-calibrated image wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits'
Saving fully-calibrated image wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits'
Preparing the HTML report for the field UMa-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01472_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257
The candidate 01472_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257 did not pass the final checks
**** FOUND 10:55:39.60 +71:52:08.5 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field UMa-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits
SExtractor catalog cache: saved UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits.cat to cache
SExtractor catalog cache: saved UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits
Creating symlink local_wcs_cache/wcs_UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits
Creating symlink local_wcs_cache/wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits
Creating symlink local_wcs_cache/wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.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_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits exists and is non-empty
wcs_UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits exists and is non-empty
wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits exists and is non-empty
wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.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 09:36:12.813 +69:59:27.41
Second-epoch image center 09:36:01.626 +69:55:46.09
Angular distance between the image centers 0.0635 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 09:36:12.813 +69:59:27.41
Second-epoch image center 09:36:03.318 +69:56:15.01
Angular distance between the image centers 0.0551 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 09:36:01.626 +69:55:46.09
Second-epoch second image center 09:36:03.318 +69:56:15.01
Angular distance between the image centers 0.00839 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/UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits &> /tmp/tmp.QxalcPLCjz
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits &> /tmp/tmp.ADDF1lUCtm
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits &> /tmp/tmp.c7ngWj1Zgx
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits &> /tmp/tmp.tbKvinayqs
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits
Calibrating the magnitude scale
Found non-empty wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.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_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits and wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.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_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits and wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits.cat
Found non-empty wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits and wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits.cat
The reference image (wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits) and catalog (wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits.cat) found
'wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits.cat' -> 'wcsmag.cat'
Read 53181 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 116.6936 to 172.5256 deg, Dec +62.8166 to +75.4852 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 116.6936 to 172.5256 deg, Dec 62.8166 to 75.4852 deg
Loaded 9539 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): 4809 out of 5497 total matches.
Matched with Tycho-2 5497 out of 53181 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.784760
a=0.000000 b=1.000000 c=22.784760
From vast_summary.log: estimated ref. image limiting mag.: -7.18
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.60
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.60
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 17 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits
2.0 pix UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits
2.4 pix fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits
2.4 pix fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits
Limiting magnitude estimates:
15.6 mag. UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits
15.6 mag. UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits
14.6 mag. fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits
14.6 mag. fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 14.0 (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.QxalcPLCjz (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits' -> 'wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits
WCS_IMAGE_NAME=wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits
WCS-calibrated image found: wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits
Checking if the catalog wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits.cat corresponding to the image wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits alredy exist and is non-empty...
Catalog wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits.cat corresponding to the image wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits
WCS catalog name: wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=2966, passed=53168
Got 53168 stars (including 50099 good ones) from the SExtractor catalog wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits.cat
util/solve_plate_with_UCAC5 got 53168 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 962 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 52713 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 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 52712 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
WARNING: Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 52712 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits -region wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.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.ADDF1lUCtm (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits' -> 'wcs_UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits
WCS_IMAGE_NAME=wcs_UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits
WCS-calibrated image found: wcs_UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits
Checking if the catalog wcs_UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits.cat corresponding to the image wcs_UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits alredy exist and is non-empty...
Catalog wcs_UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits.cat corresponding to the image wcs_UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits
WCS catalog name: wcs_UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=22, blended=2952, passed=53157
Got 53157 stars (including 50104 good ones) from the SExtractor catalog wcs_UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits.cat
util/solve_plate_with_UCAC5 got 53157 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 962 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 52771 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 764 to 829 (Dec 62.8 to 75.5)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 52772 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
WARNING: Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 52773 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits -region wcs_UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.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.c7ngWj1Zgx (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_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.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_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits
WCS_IMAGE_NAME=wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits
WCS-calibrated image found: wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits
Checking if the catalog wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits.cat corresponding to the image wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits.cat corresponding to the image wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits
WCS catalog name: wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits.cat
SExtractor catalog parsing summary: zero_flux=2, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=1914, passed=26371
Got 26371 stars (including 24417 good ones) from the SExtractor catalog wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits.cat
util/solve_plate_with_UCAC5 got 26371 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 768 to 827 (Dec 63.6 to 75.2)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 951 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 25862 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 768 to 827 (Dec 63.6 to 75.2)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 25861 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
WARNING: Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 25861 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits -region wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.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.tbKvinayqs (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_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.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_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits
WCS_IMAGE_NAME=wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits
WCS-calibrated image found: wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits
Checking if the catalog wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits.cat corresponding to the image wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits.cat corresponding to the image wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits
WCS catalog name: wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=1902, passed=26205
Got 26205 stars (including 24275 good ones) from the SExtractor catalog wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits.cat
util/solve_plate_with_UCAC5 got 26205 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 768 to 828 (Dec 63.6 to 75.2)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 955 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 25912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 768 to 828 (Dec 63.6 to 75.2)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 25911 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
WARNING: Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 25911 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits -region wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.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_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.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_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/wcs_UMa-01-Q2b1x1_2026-02-22_00-18-30_20.00sec_-15.00C_LIGHT_0264.fits
Saving fully-calibrated image wcs_UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.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_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/wcs_UMa-01-Q2b1x1_2026-02-22_00-19-18_20.00sec_-15.00C_LIGHT_0265.fits
Saving fully-calibrated image wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.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_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-47-21_20.00sec_-4.90C_LIGHT_0256.fits
Saving fully-calibrated image wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.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_2026-04-08_CI_UMa-01-Q2b1x1_054856_TTUQ2b1x1_27397_vFe8I7NX/wcs_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257.fits
Preparing the HTML report for the field UMa-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out66004.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out66529.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out66628.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out66732.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out38185.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39259.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 13s
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 66004_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257
The candidate 66004_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257 did not pass the final checks
**** FOUND 08:56:13.81 +73:50:14.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 1.361 1123973257529358720 134.05620552193 +73.83740073427 13.5913 13.0535 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.361#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 66339_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257
The candidate 66339_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257 did not pass the final checks
**** FOUND 09:10:21.87 +67:05:27.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 66529_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257
The candidate 66529_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257 did not pass the final checks
**** FOUND 11:04:51.87 +71:33:55.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 1.447 1075312858613578880 166.21634748481 +71.56493767146 13.4161 12.9278 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.447#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 66628_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257
The candidate 66628_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257 did not pass the final checks
**** FOUND 08:53:51.25 +65:24:55.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 1.348 1044684106796572672 133.46443997376 +65.41538197729 12.8005 12.1830 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.348#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 66721_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257
The candidate 66721_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257 did not pass the final checks
**** FOUND 08:46:50.47 +72:23:41.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 66732_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257
The candidate 66732_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257 did not pass the final checks
**** FOUND 09:53:21.97 +66:47:27.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 0.170 1066625720321372032 148.34153340218 +66.79093607538 13.3578 12.8434 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.170#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 66777_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257
The candidate 66777_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257 did not pass the final checks
**** FOUND 10:53:57.01 +69:52:23.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 66778_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257
The candidate 66778_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257 did not pass the final checks
**** FOUND 08:51:20.94 +73:43:59.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 66889_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257
The candidate 66889_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257 did not pass the final checks
**** FOUND 08:50:43.71 +73:45:56.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 66897_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257
The candidate 66897_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257 did not pass the final checks
**** FOUND 09:17:48.81 +69:53:16.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67002_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257
The candidate 67002_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257 did not pass the final checks
**** FOUND 09:22:45.65 +73:33:02.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67104_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257
The candidate 67104_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257 did not pass the final checks
**** FOUND 10:18:28.83 +68:02:07.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67107_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257
The candidate 67107_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257 did not pass the final checks
**** FOUND 09:34:45.39 +69:51:30.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67386_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257
The candidate 67386_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
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Considering the candidate 38185_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257
Preparing report for the candidate 38185_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257
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Considering the candidate 07659_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257
The candidate 07659_fd_UMa-01-Q2b1x1_2026-04-08_05-48-10_20.00sec_-4.90C_LIGHT_0257 did not pass the final checks