This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D
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 13.4316* 10 48 03.96 +58 57 03.4 11.5 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSV 18526,2461143.9316,11.54,0.05,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
NSV 18526 20260413.4316 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 13.4316* 10 23 17.50 +60 44 10.1 13.8 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461143.9316,13.80,0.05,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 20260413.4316 13.80CV 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: 2461083.80465266 12.02.2026 07:18:31.990 /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits
First image: 2461083.80465266 12.02.2026 07:18:31.990 /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits
Last image: 2461143.93199670 13.04.2026 10:21:54.515 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.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.: -7.45
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): 6846
Objects passed selection criteria: 6803
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 4802.5
Average stars matched: 4453 (92.7225 %)
Memory usage VmPeak: 112408 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 13 05:26:43 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: 2461083.80465266 12.02.2026 07:18:31.990 /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits
First image: 2461083.80465266 12.02.2026 07:18:31.990 /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits
Last image: 2461143.93199670 13.04.2026 10:21:54.515 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 20
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.17
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 14 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): 37532
Objects passed selection criteria: 37404
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 25874.5
Average stars matched: 24092 (93.111 %)
Memory usage VmPeak: 138636 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 13 05:27:45 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-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits
SExtractor catalog cache: saved UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits.cat to cache
SExtractor catalog cache: saved UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.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-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461143.93121711
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-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits exists and is non-empty
Saving wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits to local_wcs_cache/
'wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits' -> 'local_wcs_cache/wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits'
wcs_UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits exists and is non-empty
Saving wcs_UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits to local_wcs_cache/
'wcs_UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits' -> 'local_wcs_cache/wcs_UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits'
wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits exists and is non-empty
Saving wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits to local_wcs_cache/
'wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits' -> 'local_wcs_cache/wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits'
wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits exists and is non-empty
Saving wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits to local_wcs_cache/
'wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits' -> 'local_wcs_cache/wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.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 10:17:01.501 +61:59:55.06
Second-epoch image center 10:17:08.981 +62:00:02.08
Angular distance between the image centers 0.0148 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 10:17:01.501 +61:59:55.06
Second-epoch image center 10:17:11.694 +62:00:43.75
Angular distance between the image centers 0.0241 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 10:17:08.981 +62:00:02.08
Second-epoch second image center 10:17:11.694 +62:00:43.75
Angular distance between the image centers 0.01273 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-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits &> /tmp/tmp.KQ5W1pCxwB
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits &> /tmp/tmp.JSfJSXOiGc
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits &> /tmp/tmp.E8Uggio8pp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits &> /tmp/tmp.ScYuinnumU
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits
Calibrating the magnitude scale
Found non-empty wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.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-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits and wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.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-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits and wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits.cat
Found non-empty wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits and wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits.cat
The reference image (wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits) and catalog (wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits.cat) found
'wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits.cat' -> 'wcsmag.cat'
Read 8063 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 134.1814 to 172.7537 deg, Dec +55.2233 to +67.4954 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 134.1814 to 172.7537 deg, Dec 55.2233 to 67.4954 deg
Loaded 7313 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): 4374 out of 4626 total matches.
Matched with Tycho-2 4626 out of 8063 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.916869
a=0.000000 b=1.000000 c=22.916869
From vast_summary.log: estimated ref. image limiting mag.: -7.45
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.47
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.47
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits
2.0 pix UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits
3.1 pix fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits
3.1 pix fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits
Limiting magnitude estimates:
15.5 mag. UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits
15.5 mag. UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits
14.1 mag. fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits
14.0 mag. fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 11.6 (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.KQ5W1pCxwB (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-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.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_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.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-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.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-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits' -> 'wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits
WCS_IMAGE_NAME=wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits
WCS-calibrated image found: wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits
Checking if the catalog wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits.cat corresponding to the image wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits alredy exist and is non-empty...
Catalog wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits.cat corresponding to the image wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits
WCS catalog name: wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=579, passed=8063
Got 8063 stars (including 7472 good ones) from the SExtractor catalog wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits.cat
util/solve_plate_with_UCAC5 got 8063 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.2 to 67.5)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 970 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 7958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.2 to 67.5)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 7960 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 7960 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 978 stars left (next iteration limit 1075)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits -region wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.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.JSfJSXOiGc (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-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.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_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.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-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.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-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits' -> 'wcs_UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits
WCS_IMAGE_NAME=wcs_UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits
WCS-calibrated image found: wcs_UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits
Checking if the catalog wcs_UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits.cat corresponding to the image wcs_UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits alredy exist and is non-empty...
Catalog wcs_UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits.cat corresponding to the image wcs_UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits
WCS catalog name: wcs_UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=585, passed=8067
Got 8067 stars (including 7471 good ones) from the SExtractor catalog wcs_UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits.cat
util/solve_plate_with_UCAC5 got 8067 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.2 to 67.5)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 969 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 7961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
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 726 to 789 (Dec 55.2 to 67.5)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 7962 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 7962 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 978 stars left (next iteration limit 1075)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits -region wcs_UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.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.E8Uggio8pp (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_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.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_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits
WCS_IMAGE_NAME=wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits
WCS-calibrated image found: wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits
Checking if the catalog wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits.cat corresponding to the image wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits.cat corresponding to the image wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits
WCS catalog name: wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=298, passed=4232
Got 4232 stars (including 3930 good ones) from the SExtractor catalog wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits.cat
util/solve_plate_with_UCAC5 got 4232 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 729 to 788 (Dec 56.0 to 67.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 960 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 4119 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 56.0 to 67.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 4118 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 4118 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits -region wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.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.ScYuinnumU (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_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.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_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits
WCS_IMAGE_NAME=wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits
WCS-calibrated image found: wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits
Checking if the catalog wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits.cat corresponding to the image wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits.cat corresponding to the image wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits
WCS catalog name: wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=323, passed=4178
Got 4178 stars (including 3853 good ones) from the SExtractor catalog wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits.cat
util/solve_plate_with_UCAC5 got 4178 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (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 730 to 788 (Dec 56.1 to 67.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 962 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 4058 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 730 to 788 (Dec 56.1 to 67.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 4060 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 4060 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits -region wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.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-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits'
Saving fully-calibrated image wcs_UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/wcs_UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits'
Saving fully-calibrated image wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits'
Saving fully-calibrated image wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits'
Preparing the HTML report for the field UMa-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out01496.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21206_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566
The candidate 21206_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566 did not pass the final checks
**** FOUND 10:36:17.13 +59:56:11.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01496_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566
Preparing report for the candidate 01496_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 6s
Prepared the HTML report for the field UMa-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
10:48:03.96 +58:57:03.4
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-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits
SExtractor catalog cache: saved UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits.cat to cache
SExtractor catalog cache: saved UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.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-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits
Creating symlink local_wcs_cache/wcs_UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits
Creating symlink local_wcs_cache/wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits
Creating symlink local_wcs_cache/wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.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-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits exists and is non-empty
wcs_UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits exists and is non-empty
wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits exists and is non-empty
wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.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 10:17:01.501 +61:59:55.06
Second-epoch image center 10:17:08.981 +62:00:02.08
Angular distance between the image centers 0.0148 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 10:17:01.501 +61:59:55.06
Second-epoch image center 10:17:11.694 +62:00:43.75
Angular distance between the image centers 0.0241 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 10:17:08.981 +62:00:02.08
Second-epoch second image center 10:17:11.694 +62:00:43.75
Angular distance between the image centers 0.01273 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-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits &> /tmp/tmp.BWHl4Y0cuQ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits &> /tmp/tmp.sgEEsjrcnV
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits &> /tmp/tmp.wTDjK6l3oe
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits &> /tmp/tmp.NIqjmM1aR4
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits
Calibrating the magnitude scale
Found non-empty wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.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-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits and wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.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-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits and wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits.cat
Found non-empty wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits and wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits.cat
The reference image (wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits) and catalog (wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits.cat) found
'wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits.cat' -> 'wcsmag.cat'
Read 43866 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 134.1814 to 172.7853 deg, Dec +55.2077 to +67.4954 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 134.1814 to 172.7853 deg, Dec 55.2077 to 67.4954 deg
Loaded 7330 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): 4142 out of 4663 total matches.
Matched with Tycho-2 4663 out of 43866 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.813049
a=0.000000 b=1.000000 c=22.813049
From vast_summary.log: estimated ref. image limiting mag.: -7.17
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.64
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.64
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:
1.9 pix UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits
1.9 pix UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits
3.0 pix fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits
3.0 pix fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits
Limiting magnitude estimates:
15.6 mag. UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits
15.6 mag. UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits
14.4 mag. fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits
14.4 mag. fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 13.8 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.BWHl4Y0cuQ (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-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.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_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.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-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.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-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits' -> 'wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits
WCS_IMAGE_NAME=wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits
WCS-calibrated image found: wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits
Checking if the catalog wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits.cat corresponding to the image wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits alredy exist and is non-empty...
Catalog wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits.cat corresponding to the image wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits
WCS catalog name: wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=1995, passed=43857
Got 43857 stars (including 41793 good ones) from the SExtractor catalog wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits.cat
util/solve_plate_with_UCAC5 got 43857 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.2 to 67.5)
Done reading UCAC5 zone files...
Matched 982 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 982 matched stars entering correct_measured_positions(), 976 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 982 matched stars entering correct_measured_positions(), 43358 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
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 726 to 789 (Dec 55.2 to 67.5)
Done reading UCAC5 zone files...
Matched 982 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 982 matched stars entering correct_measured_positions(), 43359 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 982 matched stars entering correct_measured_positions(), 43359 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 982 stars left (next iteration limit 1080)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits -region wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.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.sgEEsjrcnV (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-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.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_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.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-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.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-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits' -> 'wcs_UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits
WCS_IMAGE_NAME=wcs_UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits
WCS-calibrated image found: wcs_UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits
Checking if the catalog wcs_UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits.cat corresponding to the image wcs_UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits alredy exist and is non-empty...
Catalog wcs_UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits.cat corresponding to the image wcs_UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits
WCS catalog name: wcs_UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=2030, passed=43640
Got 43640 stars (including 41530 good ones) from the SExtractor catalog wcs_UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits.cat
util/solve_plate_with_UCAC5 got 43640 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 725 to 789 (Dec 55.2 to 67.5)
Done reading UCAC5 zone files...
Matched 981 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 981 matched stars entering correct_measured_positions(), 975 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 981 matched stars entering correct_measured_positions(), 43118 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
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 725 to 789 (Dec 55.2 to 67.5)
Done reading UCAC5 zone files...
Matched 981 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 981 matched stars entering correct_measured_positions(), 43120 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 981 matched stars entering correct_measured_positions(), 43120 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 981 stars left (next iteration limit 1079)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits -region wcs_UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.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.wTDjK6l3oe (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_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.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_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits
WCS_IMAGE_NAME=wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits
WCS-calibrated image found: wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits
Checking if the catalog wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits.cat corresponding to the image wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits.cat corresponding to the image wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits
WCS catalog name: wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=1360, passed=18759
Got 18759 stars (including 17388 good ones) from the SExtractor catalog wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits.cat
util/solve_plate_with_UCAC5 got 18759 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 729 to 788 (Dec 56.0 to 67.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 957 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 18331 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 56.0 to 67.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 18332 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 18332 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits -region wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.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.NIqjmM1aR4 (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_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.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_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits
WCS_IMAGE_NAME=wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits
WCS-calibrated image found: wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits
Checking if the catalog wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits.cat corresponding to the image wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits alredy exist and is non-empty...
Catalog wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits.cat corresponding to the image wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits
WCS catalog name: wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=1635, passed=19009
Got 19009 stars (including 17363 good ones) from the SExtractor catalog wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits.cat
util/solve_plate_with_UCAC5 got 19009 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (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 730 to 788 (Dec 56.0 to 67.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 18440 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 730 to 788 (Dec 56.0 to 67.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 18438 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 18438 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits -region wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.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-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.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_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/wcs_UMa-03-Q2b1x1_2026-02-12_01-18-31_20.00sec_-14.90C_LIGHT_0318.fits
Saving fully-calibrated image wcs_UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.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_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/wcs_UMa-03-Q2b1x1_2026-02-12_01-19-21_20.00sec_-15.00C_LIGHT_0319.fits
Saving fully-calibrated image wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.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_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-20-47_20.00sec_-5.00C_LIGHT_0565.fits
Saving fully-calibrated image wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.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_2026-04-13_CI_UMa-03-Q2b1x1_052235_TTUQ2b1x1_23619_bBzaub2D/wcs_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566.fits
Preparing the HTML report for the field UMa-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_local.txt__out56211.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 21s
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 54982_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566
The candidate 54982_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566 did not pass the final checks
**** FOUND 10:47:52.53 +65:28:26.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56081_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566
The candidate 56081_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566 did not pass the final checks
**** FOUND 10:36:04.21 +63:36:12.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56211_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566
Preparing report for the candidate 56211_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566
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Considering the candidate 33657_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566
The candidate 33657_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566 did not pass the final checks
**** FOUND 09:35:34.96 +65:17:02.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 11524_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566
The candidate 11524_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566 did not pass the final checks
**** FOUND 10:36:17.12 +59:56:11.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 41548_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566
The candidate 41548_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566 did not pass the final checks
**** FOUND 10:09:07.74 +63:57:06.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 18790_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566
The candidate 18790_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566 did not pass the final checks
**** FOUND 09:55:03.57 +61:06:58.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 12302_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566
The candidate 12302_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566 did not pass the final checks
**** FOUND 10:15:07.68 +59:59:10.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 09577_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566
The candidate 09577_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566 did not pass the final checks
**** FOUND 09:58:34.17 +58:57:05.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 36583_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566
The candidate 36583_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566 did not pass the final checks
**** FOUND 09:45:55.43 +63:39:11.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 37820_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566
The candidate 37820_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566 did not pass the final checks
**** FOUND 10:18:01.57 +65:06:27.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 33369_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566
The candidate 33369_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566 did not pass the final checks
**** FOUND 09:46:03.06 +65:37:36.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 36089_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566
The candidate 36089_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566 did not pass the final checks
**** FOUND 10:24:07.59 +65:33:54.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 33903_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566
The candidate 33903_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566 did not pass the final checks
**** FOUND 09:50:23.27 +65:35:34.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 10424_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566
The candidate 10424_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566 did not pass the final checks
**** FOUND 09:50:58.90 +59:02:21.0 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 35809_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566
The candidate 35809_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566 did not pass the final checks
**** FOUND 09:44:36.40 +64:59:02.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 29731_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566
The candidate 29731_fd_UMa-03-Q2b1x1_2026-04-13_05-21-54_20.00sec_-4.90C_LIGHT_0566 did not pass the final checks