This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 04 14.0981 2461144.5981 13.21 04:30:22.38 +41:51:42.7
160.51813 -4.49684 galactic Per Second-epoch detections are separated by 6.8" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 204163714251958784 | 04:30:20.14 +41:51:45.3 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) SpType: K7 (LAMOST DR5)
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 14.0981* 04 30 22.38 +41 51 42.7 13.2 U Per 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
Large-amplitude variable Gaia DR2 204163714251958784,2461144.5981,13.21,0.05,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
Large-amplitude variable Gaia DR2 204163714251958784 20260414.0981 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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
NSVS J0458462+464203,2461144.5981,13.23,0.05,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
NSVS J0458462+464203 20260414.0981 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461083.61028419 12.02.2026 02:38:38.554 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
First image: 2461083.61028419 12.02.2026 02:38:38.554 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
Last image: 2461144.59850421 14.04.2026 02:21:40.764 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.57
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: 5 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): 20080
Objects passed selection criteria: 19996
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 15608
Average stars matched: 15147 (97.0464 %)
Memory usage VmPeak: 125976 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 13 21:27:42 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461083.61028419 12.02.2026 02:38:38.554 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
First image: 2461083.61028419 12.02.2026 02:38:38.554 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
Last image: 2461144.59850421 14.04.2026 02:21:40.764 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 119
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.23
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: 48 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): 167271
Objects passed selection criteria: 166822
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: 130086
Average stars matched: 125282 (96.3071 %)
Memory usage VmPeak: 1935492 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 13 21:31:42 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/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits
SExtractor catalog cache: saved Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits.cat to cache
SExtractor catalog cache: saved Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.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/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.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: 2461144.59767113
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits exists and is non-empty
Saving wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits to local_wcs_cache/
'wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits' -> 'local_wcs_cache/wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits'
wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits exists and is non-empty
Saving wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits to local_wcs_cache/
'wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits' -> 'local_wcs_cache/wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits'
wcs_fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits exists and is non-empty
Saving wcs_fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits to local_wcs_cache/
'wcs_fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits' -> 'local_wcs_cache/wcs_fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits'
wcs_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits exists and is non-empty
Saving wcs_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits to local_wcs_cache/
'wcs_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits' -> 'local_wcs_cache/wcs_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.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 04:48:01.099 +45:59:45.51
Second-epoch image center 04:48:01.220 +45:59:56.42
Angular distance between the image centers 0.0031 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 04:48:01.099 +45:59:45.51
Second-epoch image center 04:47:58.791 +46:00:20.10
Angular distance between the image centers 0.0117 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 04:48:01.220 +45:59:56.42
Second-epoch second image center 04:47:58.791 +46:00:20.10
Angular distance between the image centers 0.00963 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/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits &> /tmp/tmp.OhLj0Cs6R9
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits &> /tmp/tmp.4f5GJS4sqY
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits &> /tmp/tmp.B5kemay47l
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits &> /tmp/tmp.fidbCQ48l5
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits
Calibrating the magnitude scale
Found non-empty wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.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_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits and wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.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_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits and wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits.cat
Found non-empty wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits and wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits.cat
The reference image (wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits) and catalog (wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits.cat) found
'wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits.cat' -> 'wcsmag.cat'
Read 27125 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 59.9509 to 84.6314 deg, Dec +39.9814 to +51.3295 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 59.9509 to 84.6314 deg, Dec 39.9814 to 51.3295 deg
Loaded 12076 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): 8105 out of 9281 total matches.
Matched with Tycho-2 9281 out of 27125 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.966720
a=0.000000 b=1.000000 c=22.966720
From vast_summary.log: estimated ref. image limiting mag.: -7.57
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.40
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.40
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
2.0 pix Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
2.5 pix fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits
2.4 pix fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits
Limiting magnitude estimates:
15.4 mag. Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
15.4 mag. Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
14.3 mag. fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits
14.4 mag. fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 11.6 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.OhLj0Cs6R9 (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/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits' -> 'wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
WCS_IMAGE_NAME=wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
WCS-calibrated image found: wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
Checking if the catalog wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits.cat corresponding to the image wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits alredy exist and is non-empty...
Catalog wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits.cat corresponding to the image wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
WCS catalog name: wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2857, passed=27125
Got 27125 stars (including 24239 good ones) from the SExtractor catalog wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits.cat
util/solve_plate_with_UCAC5 got 27125 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 40.0 to 51.3)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 937 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 26143 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 40.0 to 51.3)
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 26143 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 26143 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits -region wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.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.4f5GJS4sqY (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/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits' -> 'wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
WCS_IMAGE_NAME=wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
WCS-calibrated image found: wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
Checking if the catalog wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits.cat corresponding to the image wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits alredy exist and is non-empty...
Catalog wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits.cat corresponding to the image wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
WCS catalog name: wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2852, passed=27075
Got 27075 stars (including 24193 good ones) from the SExtractor catalog wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits.cat
util/solve_plate_with_UCAC5 got 27075 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 40.0 to 51.3)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 934 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 25843 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 40.0 to 51.3)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 25843 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 25843 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 955 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits -region wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.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.B5kemay47l (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits
WCS_IMAGE_NAME=wcs_fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits
WCS-calibrated image found: wcs_fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits
Checking if the catalog wcs_fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits.cat corresponding to the image wcs_fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits.cat corresponding to the image wcs_fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits
WCS catalog name: wcs_fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=783, passed=11141
Got 11141 stars (including 10351 good ones) from the SExtractor catalog wcs_fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits.cat
util/solve_plate_with_UCAC5 got 11141 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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 651 to 708 (Dec 40.2 to 51.2)
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: 935 matched stars entering correct_measured_positions(), 921 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 10977 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
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 651 to 708 (Dec 40.2 to 51.2)
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: 936 matched stars entering correct_measured_positions(), 10978 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 10978 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Excluding outliers - 936 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits -region wcs_fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.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.fidbCQ48l5 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits
WCS_IMAGE_NAME=wcs_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits
WCS-calibrated image found: wcs_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits
Checking if the catalog wcs_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits.cat corresponding to the image wcs_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits.cat corresponding to the image wcs_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits
WCS catalog name: wcs_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=846, passed=11947
Got 11947 stars (including 11095 good ones) from the SExtractor catalog wcs_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits.cat
util/solve_plate_with_UCAC5 got 11947 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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 651 to 708 (Dec 40.2 to 51.3)
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: 936 matched stars entering correct_measured_positions(), 921 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 11762 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
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 651 to 708 (Dec 40.2 to 51.3)
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: 937 matched stars entering correct_measured_positions(), 11761 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 11761 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
Excluding outliers - 937 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_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits -region wcs_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.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_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits'
Saving fully-calibrated image wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits'
Saving fully-calibrated image wcs_fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/wcs_fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits'
Saving fully-calibrated image wcs_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/wcs_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits'
Preparing the HTML report for the field Per-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 31729_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 31729_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 04:34:13.03 +47:15:34.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07701_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 07701_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 04:48:11.50 +47:38:27.8 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 Per-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/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits
SExtractor catalog cache: saved Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits.cat to cache
SExtractor catalog cache: saved Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
Creating symlink local_wcs_cache/wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
Creating symlink local_wcs_cache/wcs_fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits
Creating symlink local_wcs_cache/wcs_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.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_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits exists and is non-empty
wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits exists and is non-empty
wcs_fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits exists and is non-empty
wcs_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.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 04:48:01.099 +45:59:45.51
Second-epoch image center 04:48:01.220 +45:59:56.42
Angular distance between the image centers 0.0031 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 04:48:01.099 +45:59:45.51
Second-epoch image center 04:47:58.791 +46:00:20.10
Angular distance between the image centers 0.0117 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 04:48:01.220 +45:59:56.42
Second-epoch second image center 04:47:58.791 +46:00:20.10
Angular distance between the image centers 0.00963 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/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits &> /tmp/tmp.ykMXcXHcAi
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits &> /tmp/tmp.7K1taCHwi8
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits &> /tmp/tmp.V9QUo9dUBm
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits &> /tmp/tmp.7J12UDCWVi
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits
Calibrating the magnitude scale
Found non-empty wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.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_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits and wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.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_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits and wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits.cat
Found non-empty wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits and wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits.cat
The reference image (wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits) and catalog (wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits.cat) found
'wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits.cat' -> 'wcsmag.cat'
Read 215662 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 59.9114 to 84.6651 deg, Dec +39.9364 to +51.3387 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 59.9114 to 84.6651 deg, Dec 39.9364 to 51.3387 deg
Loaded 12174 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): 6110 out of 9346 total matches.
Matched with Tycho-2 9346 out of 215662 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.835556
a=0.000000 b=1.000000 c=22.835556
From vast_summary.log: estimated ref. image limiting mag.: -7.23
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.61
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.61
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 85 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.8 pix Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
1.8 pix Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
2.4 pix fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits
2.4 pix fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits
Limiting magnitude estimates:
15.6 mag. Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
15.6 mag. Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
14.4 mag. fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits
14.5 mag. fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 13.9 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.ykMXcXHcAi (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/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits' -> 'wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
WCS_IMAGE_NAME=wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
WCS-calibrated image found: wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
Checking if the catalog wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits.cat corresponding to the image wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits alredy exist and is non-empty...
Catalog wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits.cat corresponding to the image wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
WCS catalog name: wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=60, blended=30564, passed=215602
Got 215602 stars (including 184715 good ones) from the SExtractor catalog wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits.cat
util/solve_plate_with_UCAC5 got 215602 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.3)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 949 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 211218 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.3)
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 211216 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 211216 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits -region wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.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.7K1taCHwi8 (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/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits' -> 'wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
WCS_IMAGE_NAME=wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
WCS-calibrated image found: wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
Checking if the catalog wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits.cat corresponding to the image wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits alredy exist and is non-empty...
Catalog wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits.cat corresponding to the image wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
WCS catalog name: wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=62, blended=30755, passed=215764
Got 215764 stars (including 184684 good ones) from the SExtractor catalog wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits.cat
util/solve_plate_with_UCAC5 got 215764 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.3)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 210809 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
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 649 to 708 (Dec 39.9 to 51.3)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 210809 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 210809 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits -region wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.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.V9QUo9dUBm (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits
WCS_IMAGE_NAME=wcs_fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits
WCS-calibrated image found: wcs_fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits
Checking if the catalog wcs_fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits.cat corresponding to the image wcs_fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits.cat corresponding to the image wcs_fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits
WCS catalog name: wcs_fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=7497, passed=83158
Got 83158 stars (including 75563 good ones) from the SExtractor catalog wcs_fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits.cat
util/solve_plate_with_UCAC5 got 83158 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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 651 to 708 (Dec 40.2 to 51.3)
Done reading UCAC5 zone files...
Matched 943 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(), 917 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 81489 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
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 651 to 708 (Dec 40.2 to 51.3)
Done reading UCAC5 zone files...
Matched 943 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(), 81487 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 81487 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Excluding outliers - 938 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_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits -region wcs_fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.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.7J12UDCWVi (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits
WCS_IMAGE_NAME=wcs_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits
WCS-calibrated image found: wcs_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits
Checking if the catalog wcs_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits.cat corresponding to the image wcs_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits.cat corresponding to the image wcs_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits
WCS catalog name: wcs_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=8492, passed=88673
Got 88673 stars (including 80068 good ones) from the SExtractor catalog wcs_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits.cat
util/solve_plate_with_UCAC5 got 88673 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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 651 to 708 (Dec 40.2 to 51.3)
Done reading UCAC5 zone files...
Matched 944 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(), 913 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 86812 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
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 651 to 708 (Dec 40.2 to 51.3)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 86815 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 86755 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Excluding outliers - 939 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_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits -region wcs_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.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_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
Saving fully-calibrated image wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
Saving fully-calibrated image wcs_fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/wcs_fd_Per-03-Q2b1x1_2026-04-13_21-20-28_20.00sec_-5.00C_LIGHT_0631.fits
Saving fully-calibrated image wcs_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Per-03-Q2b1x1_212311_TTUQ2b1x1_26286_Bg8yv4Ng/wcs_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632.fits
Preparing the HTML report for the field Per-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out242705.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out242713.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out242718.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out242735.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out242738.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out243592.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out243610.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out243792.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out243890.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out243894.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out243958.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out244042.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out244060.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out244068.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out244106.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out242727.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82595.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 14s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 242705_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 242705_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 05:08:01.23 +45:50:15.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 242708_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 242708_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 04:51:17.52 +43:39:21.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 242711_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 242711_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 05:06:21.23 +42:56:06.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 242713_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 242713_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 04:37:46.08 +41:51:39.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 242717_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 242717_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 04:38:55.29 +42:46:14.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 242718_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 242718_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 04:53:52.45 +42:24:10.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)GAIADR2_OUTPUT=# 1.865 204943813457494912 073.46920816437 +42.40310607897 13.5898 13.1276 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.865#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 242727_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
Preparing report for the candidate 242727_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 242730_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 242730_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 05:09:07.34 +42:07:13.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 242735_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 242735_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 05:02:30.66 +44:40:05.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 2.064 205773536717542912 075.62785052798 +44.66873550447 13.2848 12.2220 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.064#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 242737_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 242737_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 05:23:14.39 +42:04:54.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 242738_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 242738_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 05:15:22.17 +41:54:08.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 242741_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 242741_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 05:21:00.12 +43:23:55.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 242744_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 242744_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 04:50:51.87 +42:58:41.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 242748_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 242748_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 05:19:47.23 +42:06:48.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 242753_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 242753_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 04:29:40.40 +42:26:02.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 242755_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 242755_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 04:56:50.92 +42:50:53.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243272_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 243272_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 04:52:57.30 +42:34:52.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243427_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 243427_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 05:12:14.16 +45:35:50.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243498_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 243498_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 04:47:24.56 +46:00:20.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243504_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 243504_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 04:36:40.64 +45:00:57.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243520_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 243520_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 05:04:56.78 +43:20:05.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243534_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 243534_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 05:01:52.81 +43:51:42.0 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243559_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 243559_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 04:48:56.22 +43:15:33.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243565_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 243565_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 04:51:41.74 +42:03:20.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243592_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 243592_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 05:12:55.98 +42:24:27.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 1.862 201433489446972928 078.23382804814 +42.40781972916 13.1600 12.0735 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.862#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243610_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 243610_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 05:13:27.81 +43:28:17.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 0.687 202287844340762752 078.36613707690 +43.47142828501 13.3909 12.9171 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.687#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243660_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 243660_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 05:17:56.60 +46:08:22.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243676_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 243676_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 04:54:54.94 +42:57:03.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243697_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 243697_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 05:02:06.38 +43:47:10.2 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243706_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 243706_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 05:10:48.06 +46:56:04.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243723_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 243723_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 04:55:50.62 +43:08:29.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243750_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 243750_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 05:11:47.23 +45:38:45.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243755_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 243755_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 04:58:04.00 +43:14:05.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243765_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 243765_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 05:22:46.30 +47:55:39.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243773_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 243773_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 04:27:50.24 +49:27:18.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243787_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 243787_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 05:04:15.96 +45:48:22.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243792_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 243792_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 05:20:57.11 +42:20:51.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 1.963 195275738996425600 080.23722225132 +42.34773190230 13.6851 13.1609 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.963#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243800_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 243800_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 04:45:19.18 +47:28:46.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243816_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 243816_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 04:35:36.65 +45:11:49.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243829_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 243829_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 04:48:26.09 +43:18:58.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243830_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 243830_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 04:55:20.23 +43:23:43.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243844_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 243844_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 05:10:21.85 +41:54:23.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243852_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 243852_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 05:18:30.08 +47:02:13.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243881_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 243881_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 04:48:11.25 +49:31:06.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243883_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 243883_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 04:34:09.73 +45:55:33.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243890_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 243890_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 05:15:12.74 +47:11:28.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 2.639 212089268946976128 078.80383409512 +47.19188732068 13.4782 12.5899 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.639#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243894_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 243894_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 05:00:12.84 +44:53:23.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243916_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 243916_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 05:08:39.72 +42:33:23.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243923_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 243923_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 04:48:15.56 +42:48:53.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243958_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 243958_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 05:22:02.67 +48:54:17.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 2.131 213448815074231424 080.51154562474 +48.90422673832 13.9026 13.2995 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.131#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243978_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 243978_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 05:12:59.31 +44:01:12.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243982_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 243982_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 04:46:35.05 +42:20:25.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243986_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 243986_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 05:11:34.67 +49:24:08.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 243994_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 243994_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 05:01:55.64 +42:43:42.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 244006_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 244006_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 04:49:23.17 +44:13:17.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 244012_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 244012_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 04:27:48.09 +46:15:03.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 244021_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 244021_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 04:51:11.69 +48:42:42.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 244042_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 244042_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 05:09:05.73 +43:01:07.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 5.102 202261078105129088 077.27197220671 +43.01834006046 13.9488 13.3318 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.102#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 244059_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 244059_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 04:40:04.70 +43:16:56.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 244060_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 244060_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 05:20:37.89 +43:07:53.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 3.296 207332060091272960 080.15863211225 +43.13231349784 13.7794 12.9852 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.296#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 244068_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 244068_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 05:05:27.97 +46:56:39.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 2.828 207038524845889280 076.36760790051 +46.94451765731 13.8880 13.2692 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.828#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 244073_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 244073_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 05:08:58.47 +44:38:36.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 244106_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 244106_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 05:23:01.23 +42:34:56.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 3.362 195261204826052480 080.75610223872 +42.58298434128 14.0489 13.5524 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.362#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 244145_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 244145_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 04:58:01.53 +49:10:32.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 244163_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 244163_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 05:07:33.85 +46:59:42.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 244170_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 244170_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 05:24:34.96 +45:25:42.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 244191_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 244191_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 05:10:25.18 +45:27:19.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 244211_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 244211_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 04:49:41.85 +46:32:13.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 244232_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 244232_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 04:48:58.07 +43:58:00.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 244241_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 244241_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 04:55:20.88 +44:06:44.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 244295_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 244295_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 04:47:57.47 +45:28:15.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 244318_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 244318_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 05:23:22.89 +42:22:13.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 244336_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 244336_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 244385_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 244385_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 04:48:35.62 +43:45:58.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 244390_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 244390_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 05:10:00.72 +46:00:33.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 172015_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 172015_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 04:27:32.52 +41:47:05.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23829_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 23829_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 04:25:56.41 +49:53:23.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 75612_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 75612_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 04:34:13.04 +47:15:34.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86766_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 86766_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 04:38:30.87 +46:40:08.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 82595_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
Preparing report for the candidate 82595_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22973_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 22973_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 04:54:15.02 +49:53:59.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58320_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 58320_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 04:33:44.11 +48:06:52.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 82979_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 82979_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 05:04:11.63 +46:36:31.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68436_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 68436_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks
**** FOUND 04:48:11.49 +47:38:27.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28761_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632
The candidate 28761_fd_Per-03-Q2b1x1_2026-04-13_21-21-40_20.00sec_-4.90C_LIGHT_0632 did not pass the final checks