This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x
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 09.1387* 05 15 05.26 +06 18 59.0 12.8 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461139.6387,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260409.1387 12.77CV 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 09.1387* 05 17 23.33 +03 53 24.2 13.8 U Ori 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
Gaia DR3 3235540808452398208,2461139.6387,13.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3235540808452398208 20260409.1387 13.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.68831204 09.01.2026 04:31:00.160 /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
First image: 2461049.68831204 09.01.2026 04:31:00.160 /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
Last image: 2461139.63903252 09.04.2026 03:20:02.410 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.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.: -7.61
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: 7 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): 13534
Objects passed selection criteria: 13485
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 9731.75
Average stars matched: 8848.75 (90.9266 %)
Memory usage VmPeak: 117852 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Apr 8 23:44:10 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.68831204 09.01.2026 04:31:00.160 /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
First image: 2461049.68831204 09.01.2026 04:31:00.160 /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
Last image: 2461139.63903252 09.04.2026 03:20:02.410 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 44
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.26
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: 36 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): 87654
Objects passed selection criteria: 87417
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 67420.8
Average stars matched: 61942.8 (91.8749 %)
Memory usage VmPeak: 2065044 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Apr 8 23:45:52 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/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits
SExtractor catalog cache: saved Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits.cat to cache
SExtractor catalog cache: saved Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.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/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.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: 2461139.63846638
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_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits exists and is non-empty
Saving wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits to local_wcs_cache/
'wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits' -> 'local_wcs_cache/wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits'
wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits exists and is non-empty
Saving wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits to local_wcs_cache/
'wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits' -> 'local_wcs_cache/wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits'
wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits exists and is non-empty
Saving wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits to local_wcs_cache/
'wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits' -> 'local_wcs_cache/wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits'
wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits exists and is non-empty
Saving wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits to local_wcs_cache/
'wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits' -> 'local_wcs_cache/wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:08:30.148 +06:00:49.89
Second-epoch image center 05:08:34.492 +06:00:13.03
Angular distance between the image centers 0.0207 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:08:30.148 +06:00:49.89
Second-epoch image center 05:08:33.434 +05:59:53.28
Angular distance between the image centers 0.0208 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 05:08:34.492 +06:00:13.03
Second-epoch second image center 05:08:33.434 +05:59:53.28
Angular distance between the image centers 0.00702 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/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits &> /tmp/tmp.is9qnOd1CR
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits &> /tmp/tmp.SeQkLNdJv1
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits &> /tmp/tmp.pV3kpbiVIR
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits &> /tmp/tmp.T6u7dwyLrK
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits
Calibrating the magnitude scale
Found non-empty wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.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_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits and wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.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_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits and wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits.cat
Found non-empty wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits and wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits.cat
The reference image (wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits) and catalog (wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits.cat) found
'wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits.cat' -> 'wcsmag.cat'
Read 16511 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 69.0486 to 85.0652 deg, Dec +0.5907 to +11.3430 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 69.0486 to 85.0652 deg, Dec 0.5907 to 11.3430 deg
Loaded 9689 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): 7647 out of 8333 total matches.
Matched with Tycho-2 8333 out of 16511 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.928470
a=0.000000 b=1.000000 c=22.928470
From vast_summary.log: estimated ref. image limiting mag.: -7.61
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.32
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.32
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 Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
2.0 pix Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
2.7 pix fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits
2.7 pix fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits
Limiting magnitude estimates:
15.3 mag. Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
15.3 mag. Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
14.4 mag. fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits
14.4 mag. fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 11.5 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.is9qnOd1CR (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/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits' -> 'wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
WCS_IMAGE_NAME=wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
WCS-calibrated image found: wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
Checking if the catalog wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits.cat corresponding to the image wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits alredy exist and is non-empty...
Catalog wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits.cat corresponding to the image wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
WCS catalog name: wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1518, passed=16511
Got 16511 stars (including 14968 good ones) from the SExtractor catalog wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits.cat
util/solve_plate_with_UCAC5 got 16511 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 916 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 15824 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
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 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 15825 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 15825 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 946 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits -region wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.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.SeQkLNdJv1 (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/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits' -> 'wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
WCS_IMAGE_NAME=wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
WCS-calibrated image found: wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
Checking if the catalog wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits.cat corresponding to the image wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits alredy exist and is non-empty...
Catalog wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits.cat corresponding to the image wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
WCS catalog name: wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1534, passed=16525
Got 16525 stars (including 14970 good ones) from the SExtractor catalog wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits.cat
util/solve_plate_with_UCAC5 got 16525 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.4)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 917 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 15900 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.4)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 15898 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 15898 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits -region wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.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.pV3kpbiVIR (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits
WCS_IMAGE_NAME=wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits
WCS-calibrated image found: wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits
Checking if the catalog wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits.cat corresponding to the image wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits.cat corresponding to the image wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits
WCS catalog name: wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=654, passed=9575
Got 9575 stars (including 8915 good ones) from the SExtractor catalog wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits.cat
util/solve_plate_with_UCAC5 got 9575 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (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 0.010422 (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 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 931 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 9426 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
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 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 9426 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 9426 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 936 stars left (next iteration limit 1030)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits -region wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.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.T6u7dwyLrK (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits
WCS_IMAGE_NAME=wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits
WCS-calibrated image found: wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits
Checking if the catalog wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits.cat corresponding to the image wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits.cat corresponding to the image wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits
WCS catalog name: wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=663, passed=9501
Got 9501 stars (including 8824 good ones) from the SExtractor catalog wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits.cat
util/solve_plate_with_UCAC5 got 9501 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (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 0.010422 (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 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 929 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 9343 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
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 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 9342 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 9342 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Excluding outliers - 936 stars left (next iteration limit 1029)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits -region wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.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_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits'
Saving fully-calibrated image wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits'
Saving fully-calibrated image wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits'
Saving fully-calibrated image wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits'
Preparing the HTML report for the field Ori-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21930_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087
The candidate 21930_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 04:54:23.45 +07:50:23.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11747_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087
The candidate 11747_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 04:59:00.59 +08:07:49.3 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Ori-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits
SExtractor catalog cache: saved Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits.cat to cache
SExtractor catalog cache: saved Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
Creating symlink local_wcs_cache/wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
Creating symlink local_wcs_cache/wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits
Creating symlink local_wcs_cache/wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.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_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits exists and is non-empty
wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits exists and is non-empty
wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits exists and is non-empty
wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:08:30.148 +06:00:49.89
Second-epoch image center 05:08:34.492 +06:00:13.03
Angular distance between the image centers 0.0207 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:08:30.148 +06:00:49.89
Second-epoch image center 05:08:33.434 +05:59:53.28
Angular distance between the image centers 0.0208 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 05:08:34.492 +06:00:13.03
Second-epoch second image center 05:08:33.434 +05:59:53.28
Angular distance between the image centers 0.00702 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/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits &> /tmp/tmp.nvmNwNGoK5
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits &> /tmp/tmp.rGmSG04CMX
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits &> /tmp/tmp.zawWLNxoNW
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits &> /tmp/tmp.6ORLcynqkK
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits
Calibrating the magnitude scale
Found non-empty wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.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_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits and wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.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_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits and wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits.cat
Found non-empty wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits and wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits.cat
The reference image (wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits) and catalog (wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits.cat) found
'wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits.cat' -> 'wcsmag.cat'
Read 107661 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 69.0344 to 85.0658 deg, Dec +0.5907 to +11.3441 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 69.0344 to 85.0658 deg, Dec 0.5907 to 11.3441 deg
Loaded 9691 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): 6705 out of 8494 total matches.
Matched with Tycho-2 8494 out of 107661 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.790183
a=0.000000 b=1.000000 c=22.790183
From vast_summary.log: estimated ref. image limiting mag.: -7.26
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.53
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.53
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 38 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
1.9 pix Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
2.2 pix fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits
2.2 pix fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits
Limiting magnitude estimates:
15.5 mag. Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
15.5 mag. Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
14.6 mag. fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits
14.6 mag. fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 14.2 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.nvmNwNGoK5 (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/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits' -> 'wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
WCS_IMAGE_NAME=wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
WCS-calibrated image found: wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
Checking if the catalog wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits.cat corresponding to the image wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits alredy exist and is non-empty...
Catalog wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits.cat corresponding to the image wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
WCS catalog name: wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=27, blended=9183, passed=107634
Got 107634 stars (including 98272 good ones) from the SExtractor catalog wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits.cat
util/solve_plate_with_UCAC5 got 107634 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 922 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 103134 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
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 452 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 103131 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 103130 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 949 stars left (next iteration limit 1043)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits -region wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.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.rGmSG04CMX (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/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits' -> 'wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
WCS_IMAGE_NAME=wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
WCS-calibrated image found: wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
Checking if the catalog wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits.cat corresponding to the image wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits alredy exist and is non-empty...
Catalog wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits.cat corresponding to the image wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
WCS catalog name: wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=33, blended=9161, passed=107847
Got 107847 stars (including 98493 good ones) from the SExtractor catalog wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits.cat
util/solve_plate_with_UCAC5 got 107847 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.4)
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 917 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 104030 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.4)
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 104032 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 104028 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 946 stars left (next iteration limit 1041)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits -region wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.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.zawWLNxoNW (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits
WCS_IMAGE_NAME=wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits
WCS-calibrated image found: wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits
Checking if the catalog wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits.cat corresponding to the image wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits.cat corresponding to the image wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits
WCS catalog name: wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=3809, passed=61024
Got 61024 stars (including 57146 good ones) from the SExtractor catalog wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits.cat
util/solve_plate_with_UCAC5 got 61024 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (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 0.010422 (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 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 60190 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
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 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 60190 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 60190 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 938 stars left (next iteration limit 1032)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits -region wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.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.6ORLcynqkK (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits
WCS_IMAGE_NAME=wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits
WCS-calibrated image found: wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits
Checking if the catalog wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits.cat corresponding to the image wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits.cat corresponding to the image wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits
WCS catalog name: wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=33, blended=3861, passed=61436
Got 61436 stars (including 57497 good ones) from the SExtractor catalog wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits.cat
util/solve_plate_with_UCAC5 got 61436 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (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 0.010422 (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 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 929 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 60460 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
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 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 60462 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Accuracy estimation diagnostic: 940 matched stars entering correct_measured_positions(), 60461 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Excluding outliers - 940 stars left (next iteration limit 1032)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits -region wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.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_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
Saving fully-calibrated image wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
Saving fully-calibrated image wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-19-13_20.00sec_-5.00C_LIGHT_0086.fits
Saving fully-calibrated image wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Ori-03-Q2b1x1_232728_TTUQ2b1x1_22852_D91rfw1x/wcs_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087.fits
Preparing the HTML report for the field Ori-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out124391.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124395.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124404.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124409.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134904.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out136129.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out129336.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134656.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 124391_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087
The candidate 124391_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 05:03:37.34 +06:10:58.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.52, MAG_FAINT_SEARCH_LIMIT=15.50)GAIADR2_OUTPUT=# 0.803 3240206929643430656 075.90545559476 +06.18276110071 14.5973 14.1228 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.803#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124395_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087
The candidate 124395_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 04:58:59.82 +07:44:38.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.54, MAG_FAINT_SEARCH_LIMIT=15.52)GAIADR2_OUTPUT=# 2.112 3288666736406694912 074.74929251549 +07.74330374120 14.9236 14.3715 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.112#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124404_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087
The candidate 124404_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 05:20:29.62 +10:16:33.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.22, MAG_FAINT_SEARCH_LIMIT=15.20)GAIADR2_OUTPUT=# 2.053 3338822299336452992 080.12305505839 +10.27560990245 14.1308 13.4498 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.053#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124409_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087
The candidate 124409_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 05:00:35.27 +04:37:38.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 0.592 3239386075494081536 075.14681751770 +04.62727531516 13.7802 13.2859 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.592#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124414_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087
The candidate 124414_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 04:51:53.45 +08:50:28.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 124416_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087
The candidate 124416_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 05:25:21.33 +08:24:21.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 124420_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087
The candidate 124420_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 05:26:13.40 +09:06:41.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 124422_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087
The candidate 124422_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 05:22:05.62 +02:19:12.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 124425_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087
The candidate 124425_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 05:01:01.51 +07:07:33.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 124427_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087
The candidate 124427_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 05:17:24.35 +03:53:22.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 127609_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087
The candidate 127609_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 04:54:54.99 +10:11:07.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 128668_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087
The candidate 128668_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 05:20:59.65 +09:43:43.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 129336_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087
Preparing report for the candidate 129336_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087
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Considering the candidate 130536_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087
The candidate 130536_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 05:15:10.21 +03:28:39.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 131276_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087
The candidate 131276_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 05:11:45.06 +05:23:35.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 131499_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087
The candidate 131499_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 04:52:57.22 +07:45:23.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 131737_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087
The candidate 131737_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 04:53:09.81 +08:33:59.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 131858_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087
The candidate 131858_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 05:25:05.31 +09:59:24.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 131978_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087
The candidate 131978_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 05:00:09.01 +03:15:15.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 132822_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087
The candidate 132822_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 05:22:42.21 +03:32:48.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 132930_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087
The candidate 132930_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 04:56:44.04 +08:50:29.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 133178_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087
The candidate 133178_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 05:05:09.37 +08:57:20.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 133555_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087
The candidate 133555_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 05:01:08.65 +07:51:53.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 133623_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087
The candidate 133623_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 05:02:34.08 +03:26:16.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 133710_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087
The candidate 133710_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 04:51:20.18 +05:35:26.9 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 134548_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087
The candidate 134548_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 05:06:59.22 +07:26:52.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 134610_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087
The candidate 134610_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 05:08:53.57 +03:11:51.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 134656_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087
Preparing report for the candidate 134656_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087
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Considering the candidate 134904_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087
The candidate 134904_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 05:02:06.19 +03:13:08.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 3.445 3238192967938755072 075.52558142186 +03.21795531579 14.2936 13.8472 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.445#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 134983_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087
The candidate 134983_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 05:03:41.27 +06:37:27.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 135374_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087
The candidate 135374_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 05:11:23.45 +05:42:40.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 135773_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087
The candidate 135773_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 04:52:09.13 +06:28:26.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 136125_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087
The candidate 136125_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 04:54:39.72 +07:47:34.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 136129_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087
The candidate 136129_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 05:01:48.81 +08:27:26.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 2.366 3290221033530491904 075.45309512455 +08.45679266322 14.2233 13.7530 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.366#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 136206_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087
The candidate 136206_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 05:01:49.38 +06:44:32.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 138031_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087
The candidate 138031_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 05:02:21.24 +05:29:23.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 119019_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087
The candidate 119019_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks
**** FOUND 04:54:23.30 +07:50:21.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101230_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087
The candidate 101230_fd_Ori-03-Q2b1x1_2026-04-08_22-20-02_20.00sec_-4.90C_LIGHT_0087 did not pass the final checks