This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 11.1945* 03 19 00.51 +34 26 23.1 13.3 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461082.6945,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260211.1945 13.30CV 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
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:19:00.51 +34:26:23.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20_00sec_-15_00C_LIGHT_0297_fits__*pix.png resample_wcs_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20_00sec_-14_90C_LIGHT_0148_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20_00sec_-15_00C_LIGHT_0297_fits__*pix.png resample_wcs_fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20_00sec_-14_90C_LIGHT_0147_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20_00sec_-15_00C_LIGHT_0297_fits__*pix.png resample_wcs_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20_00sec_-14_90C_LIGHT_0148_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20_00sec_-15_00C_LIGHT_0297_fits__*pix.png resample_wcs_fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20_00sec_-14_90C_LIGHT_0147_fits__*pix.png animation_v2.gif
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 02 11.1945* 03 51 15.18 +33 02 13.8 13.1 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
RX Per,2461082.6945,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
RX Per 20260211.1945 13.13CV 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
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:51:15.18 +33:02:13.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20_00sec_-15_00C_LIGHT_0297_fits__*pix.png resample_wcs_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20_00sec_-14_90C_LIGHT_0148_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20_00sec_-15_00C_LIGHT_0297_fits__*pix.png resample_wcs_fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20_00sec_-14_90C_LIGHT_0147_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20_00sec_-15_00C_LIGHT_0297_fits__*pix.png resample_wcs_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20_00sec_-14_90C_LIGHT_0148_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20_00sec_-15_00C_LIGHT_0297_fits__*pix.png resample_wcs_fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20_00sec_-14_90C_LIGHT_0147_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.76090821 23.12.2025 06:15:32.469 /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits
First image: 2461032.76090821 23.12.2025 06:15:32.469 /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits
Last image: 2461082.69478936 11.02.2026 04:40:19.801 /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 15
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.55
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 7 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 18732
Objects passed selection criteria: 18717
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 17892.5
Average stars matched: 17602.5 (98.3792 %)
Memory usage VmPeak: 123124 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Tue Feb 10 15:05:05 CST 2026
VaST build number 1.0rc88-299-g877bacc0
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Feb 10 22:57:41 CST 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: 2461032.76090821 23.12.2025 06:15:32.469 /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits
First image: 2461032.76090821 23.12.2025 06:15:32.469 /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits
Last image: 2461082.69478936 11.02.2026 04:40:19.801 /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 172
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.25
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: 102 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): 125220
Objects passed selection criteria: 124955
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 118828
Average stars matched: 115371 (97.0908 %)
Memory usage VmPeak: 1905120 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Tue Feb 10 15:05:05 CST 2026
VaST build number 1.0rc88-299-g877bacc0
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Feb 10 23:00:56 CST 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits
SExtractor catalog cache: saved Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits.cat to cache
SExtractor catalog cache: saved Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.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-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.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: 2461082.69417016
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits exists and is non-empty
Saving wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits to local_wcs_cache/
'wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits' -> 'local_wcs_cache/wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits'
wcs_Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits exists and is non-empty
Saving wcs_Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits to local_wcs_cache/
'wcs_Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits' -> 'local_wcs_cache/wcs_Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits'
wcs_fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits exists and is non-empty
Saving wcs_fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits to local_wcs_cache/
'wcs_fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits' -> 'local_wcs_cache/wcs_fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits'
wcs_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits exists and is non-empty
Saving wcs_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits to local_wcs_cache/
'wcs_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits' -> 'local_wcs_cache/wcs_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.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 03:16:22.391 +37:59:55.30
Second-epoch image center 03:16:22.868 +37:59:54.68
Angular distance between the image centers 0.00 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 03:16:22.391 +37:59:55.30
Second-epoch image center 03:16:20.369 +38:00:35.80
Angular distance between the image centers 0.01 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 03:16:22.868 +37:59:54.68
Second-epoch second image center 03:16:20.369 +38:00:35.80
Angular distance between the image centers 0.01406 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-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits &> /tmp/tmp.hvzZL4n0U4
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits &> /tmp/tmp.sQEg8Su0jU
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits &> /tmp/tmp.rgI13WkhOx
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits &> /tmp/tmp.9yn0sTrZUa
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits
Calibrating the magnitude scale
Found non-empty wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.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-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits and wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.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-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits and wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits.cat
Found non-empty wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits and wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits.cat
The reference image (wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits) and catalog (wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits.cat) found
'wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits.cat' -> 'wcsmag.cat'
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
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 9105 out of 19456 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.946435
a=0.000000 b=1.000000 c=22.946435
From vast_summary.log: estimated ref. image limiting mag.: -7.55
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
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 15 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits
2.0 pix Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits
2.4 pix fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits
2.4 pix fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits
Limiting magnitude estimates:
15.4 mag. Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits
15.4 mag. Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits
15.1 mag. fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits
15.1 mag. fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 12.2 (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 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.hvzZL4n0U4 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.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-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits' -> 'wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits
WCS_IMAGE_NAME=wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits
WCS-calibrated image found: wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits
Checking if the catalog wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits.cat corresponding to the image wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits alredy exist and is non-empty...
Catalog wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits.cat corresponding to the image wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits
WCS catalog name: wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1692, passed=19456
Got 19456 stars (including 17731 good ones) from the SExtractor catalog wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits.cat
util/solve_plate_with_UCAC5 got 19456 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.36"
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits -region wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.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.sQEg8Su0jU (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.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-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits' -> 'wcs_Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits
WCS_IMAGE_NAME=wcs_Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits
WCS-calibrated image found: wcs_Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits
Checking if the catalog wcs_Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits.cat corresponding to the image wcs_Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits alredy exist and is non-empty...
Catalog wcs_Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits.cat corresponding to the image wcs_Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits
WCS catalog name: wcs_Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1678, passed=19305
Got 19305 stars (including 17598 good ones) from the SExtractor catalog wcs_Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits.cat
util/solve_plate_with_UCAC5 got 19305 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
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...
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.37"
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits -region wcs_Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.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.rgI13WkhOx (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_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.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_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits
WCS_IMAGE_NAME=wcs_fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits
WCS-calibrated image found: wcs_fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits
Checking if the catalog wcs_fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits.cat corresponding to the image wcs_fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits.cat corresponding to the image wcs_fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits
WCS catalog name: wcs_fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1419, passed=16676
Got 16676 stars (including 15233 good ones) from the SExtractor catalog wcs_fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits.cat
util/solve_plate_with_UCAC5 got 16676 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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...
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.43"
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 953 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits -region wcs_fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.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.9yn0sTrZUa (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_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.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_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits
WCS_IMAGE_NAME=wcs_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits
WCS-calibrated image found: wcs_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits
Checking if the catalog wcs_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits.cat corresponding to the image wcs_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits.cat corresponding to the image wcs_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits
WCS catalog name: wcs_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1392, passed=16539
Got 16539 stars (including 15125 good ones) from the SExtractor catalog wcs_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits.cat
util/solve_plate_with_UCAC5 got 16539 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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...
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.43"
Estimated accuracy of the plate solution: 0.45"
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_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits -region wcs_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.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_fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/wcs_fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits'
Saving fully-calibrated image wcs_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/wcs_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits'
Preparing the HTML report for the field Per-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20976.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20955_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 20955_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 03:43:41.41 +33:31:03.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20956_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 20956_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 03:39:23.28 +41:52:54.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20961_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 20961_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 02:59:56.36 +42:37:13.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20967_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 20967_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 02:52:26.01 +36:41:29.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20969_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 20969_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 03:14:39.64 +33:18:08.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20976_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 20976_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 03:23:46.77 +40:37:40.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 3.166 236309998277118464 050.94371646336 +40.62790494227 12.1889 11.7181 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.166#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20980_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 20980_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 03:30:36.01 +37:18:48.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20983_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 20983_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 03:50:13.90 +35:36:45.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20984_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 20984_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 03:41:50.98 +41:59:17.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20986_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 20986_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 03:07:36.57 +42:54:07.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20988_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 20988_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 03:46:54.82 +37:29:22.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20991_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 20991_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 03:22:04.64 +42:12:32.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20995_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 20995_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 03:41:32.42 +38:12:57.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20998_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 20998_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 03:29:22.38 +39:29:18.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14985_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 14985_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 03:30:03.07 +35:40:16.5 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Per-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits
SExtractor catalog cache: saved Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits.cat to cache
SExtractor catalog cache: saved Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.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-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits
Creating symlink local_wcs_cache/wcs_Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits
Creating symlink local_wcs_cache/wcs_fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits
Creating symlink local_wcs_cache/wcs_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.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-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits exists and is non-empty
wcs_Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits exists and is non-empty
wcs_fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits exists and is non-empty
wcs_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.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 03:16:22.391 +37:59:55.30
Second-epoch image center 03:16:22.868 +37:59:54.68
Angular distance between the image centers 0.00 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 03:16:22.391 +37:59:55.30
Second-epoch image center 03:16:20.369 +38:00:35.80
Angular distance between the image centers 0.01 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 03:16:22.868 +37:59:54.68
Second-epoch second image center 03:16:20.369 +38:00:35.80
Angular distance between the image centers 0.01406 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-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits &> /tmp/tmp.sYrQHjkg79
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits &> /tmp/tmp.GnESlpRykn
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits &> /tmp/tmp.LZRNrSyJhJ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits &> /tmp/tmp.D0lNmVjFiN
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits
Calibrating the magnitude scale
Found non-empty wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.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-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits and wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.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-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits and wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits.cat
Found non-empty wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits and wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits.cat
The reference image (wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits) and catalog (wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits.cat) found
'wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits.cat' -> 'wcsmag.cat'
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
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 9215 out of 130207 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.812433
a=0.000000 b=1.000000 c=22.812433
From vast_summary.log: estimated ref. image limiting mag.: -7.25
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.56
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.56
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 65 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits
1.9 pix Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits
2.2 pix fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits
2.2 pix fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits
Limiting magnitude estimates:
15.6 mag. Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits
15.6 mag. Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits
15.3 mag. fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits
15.3 mag. fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits
All-image limiting magnitude estimate: 15.3 (SNR ) 14.6 (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 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.sYrQHjkg79 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.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-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits' -> 'wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits
WCS_IMAGE_NAME=wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits
WCS-calibrated image found: wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits
Checking if the catalog wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits.cat corresponding to the image wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits alredy exist and is non-empty...
Catalog wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits.cat corresponding to the image wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits
WCS catalog name: wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=29, blended=13125, passed=130178
Got 130178 stars (including 116858 good ones) from the SExtractor catalog wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits.cat
util/solve_plate_with_UCAC5 got 130178 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
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...
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.37"
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 958 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits -region wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-04-Q1b1x1_2025-12-23_00-15-32_20.00sec_-15.00C_LIGHT_0297.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.GnESlpRykn (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.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-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits' -> 'wcs_Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits
WCS_IMAGE_NAME=wcs_Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits
WCS-calibrated image found: wcs_Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits
Checking if the catalog wcs_Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits.cat corresponding to the image wcs_Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits alredy exist and is non-empty...
Catalog wcs_Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits.cat corresponding to the image wcs_Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits
WCS catalog name: wcs_Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=54, blended=13105, passed=131471
Got 131471 stars (including 118167 good ones) from the SExtractor catalog wcs_Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits.cat
util/solve_plate_with_UCAC5 got 131471 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
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...
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
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...
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.37"
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-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits -region wcs_Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-04-Q1b1x1_2025-12-23_00-16-14_20.00sec_-15.00C_LIGHT_0298.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.LZRNrSyJhJ (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_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.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_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits
WCS_IMAGE_NAME=wcs_fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits
WCS-calibrated image found: wcs_fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits
Checking if the catalog wcs_fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits.cat corresponding to the image wcs_fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits.cat corresponding to the image wcs_fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits
WCS catalog name: wcs_fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=23, blended=10710, passed=108384
Got 108384 stars (including 97500 good ones) from the SExtractor catalog wcs_fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits.cat
util/solve_plate_with_UCAC5 got 108384 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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...
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.44"
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 954 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_fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits -region wcs_fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.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.D0lNmVjFiN (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_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.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_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits
WCS_IMAGE_NAME=wcs_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits
WCS-calibrated image found: wcs_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits
Checking if the catalog wcs_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits.cat corresponding to the image wcs_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits.cat corresponding to the image wcs_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits
WCS catalog name: wcs_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=30, blended=10569, passed=108375
Got 108375 stars (including 97641 good ones) from the SExtractor catalog wcs_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits.cat
util/solve_plate_with_UCAC5 got 108375 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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...
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.43"
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 957 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_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits -region wcs_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.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_fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.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_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/wcs_fd_Per-04-Q1b1x1_2026-02-10_22-39-26_20.00sec_-14.90C_LIGHT_0147.fits
Saving fully-calibrated image wcs_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.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_2026-02-10_CI_Per-04-Q1b1x1_225518_TTUQ1b1x1_26038_6PjDdTHI/wcs_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148.fits
Preparing the HTML report for the field Per-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out151546.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151555.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151556.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151559.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151561.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151582.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151587.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151591.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151594.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151601.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151615.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151618.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151619.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151630.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151631.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151632.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151634.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151638.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151667.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151687.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151725.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151736.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151740.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151751.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151766.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151786.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151804.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151825.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out151865.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out151701.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out96112.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 11s
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 151537_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151537_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 03:19:59.83 +42:49:25.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151546_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151546_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 02:41:42.83 +40:32:25.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 1.348 335165783059730432 040.42842114301 +40.54079011648 14.6988 14.0407 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.348#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151555_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151555_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 02:57:05.70 +40:03:49.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 0.888 143866977623103488 044.27395668991 +40.06364404192 14.5665 14.0983 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.888#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151556_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151556_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 03:54:20.57 +40:57:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)GAIADR2_OUTPUT=# 1.300 230194823841500288 058.58606606989 +40.95153817968 14.4630 13.7025 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.300#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151559_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151559_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 02:37:26.79 +41:52:38.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)GAIADR2_OUTPUT=# 3.865 340022188481431936 039.36142198534 +41.87638140053 14.9251 14.4397 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.865#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151561_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151561_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 02:56:58.67 +39:31:06.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.45, MAG_FAINT_SEARCH_LIMIT=15.43)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151562_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151562_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151572_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151572_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 02:44:46.74 +41:39:25.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151582_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151582_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 03:35:20.88 +40:51:28.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151587_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151587_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 02:35:52.50 +42:41:24.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151591_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151591_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 03:02:36.94 +36:27:34.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 1.607 141910637199181952 045.65402263704 +36.45925634613 14.1389 13.6312 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.607#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151594_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151594_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 03:03:06.21 +34:01:38.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.09, MAG_FAINT_SEARCH_LIMIT=15.07)GAIADR2_OUTPUT=# 0.990 136966648805115648 045.77578203288 +34.02751396810 13.8728 13.1843 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.990#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151595_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151595_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 02:42:13.51 +41:44:12.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151598_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151598_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 02:57:02.91 +38:13:32.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151599_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151599_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 02:48:53.95 +41:56:35.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151601_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151601_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 02:49:37.16 +39:28:52.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)GAIADR2_OUTPUT=# 0.702 335574767025164800 042.40490213231 +39.48103446755 13.9366 13.3697 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.702#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151602_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151602_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 03:03:03.35 +42:56:23.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151609_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151609_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 02:53:48.96 +41:51:37.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151611_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151611_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 02:55:42.12 +42:43:16.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151614_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151614_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 03:24:01.94 +42:45:20.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151615_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151615_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 03:07:42.62 +39:05:46.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 0.560 142696891092361344 046.92756059104 +39.09606768082 13.8423 13.2739 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.560#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151616_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151616_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 03:02:57.01 +42:24:02.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151617_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151617_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 02:37:19.32 +41:55:50.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151618_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151618_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 02:42:04.20 +36:05:17.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151619_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151619_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 02:59:36.84 +33:47:57.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 1.086 136922256022892544 044.90336517006 +33.79908099379 13.9456 13.3816 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.086#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151621_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151621_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 02:49:22.91 +41:40:53.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151622_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151622_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 02:41:54.57 +38:59:22.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151625_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151625_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 02:38:34.34 +36:54:09.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151630_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151630_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 03:00:30.05 +40:19:28.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 1.005 143788946656832640 045.12508112711 +40.32492840062 13.4271 12.6639 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.005#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151631_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151631_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 02:46:55.27 +41:46:55.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 1.560 336840270549027328 041.72988482247 +41.78242042987 13.5265 13.0241 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.560#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151632_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151632_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 03:00:58.03 +41:04:17.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 0.501 144031457690469504 045.24186079891 +41.07139864321 13.4191 12.7705 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.501#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151634_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151634_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 02:52:43.74 +39:14:26.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151635_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151635_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 02:47:45.48 +38:24:11.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151636_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151636_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 02:41:39.23 +38:39:37.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151638_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151638_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 02:42:29.01 +42:17:02.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 0.739 337091062279687296 040.62098963786 +42.28415906721 13.1806 12.5844 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.739#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151667_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151667_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 02:48:19.31 +42:57:49.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 0.624 337332920477958272 042.08055393700 +42.96379741596 12.9295 12.4289 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.624#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151669_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151669_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 03:07:36.48 +42:54:07.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151670_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151670_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 02:59:10.62 +36:10:38.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151684_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151684_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 02:40:30.29 +35:02:32.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151687_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151687_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 02:49:55.47 +33:06:49.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 0.633 139622759660108288 042.48094089595 +33.11363773063 12.9388 12.4591 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.633#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151701_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
Preparing report for the candidate 151701_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151722_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151722_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 02:48:21.25 +38:26:37.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151725_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151725_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 02:45:36.88 +34:39:50.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 1.526 140020507991643008 041.40317631267 +34.66407468656 13.8173 13.3266 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.526#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151736_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151736_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 02:58:53.62 +35:11:45.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 5.232 137320034419920512 044.72176125531 +35.19535794337 13.6904 12.9643 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.232#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151740_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151740_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 02:39:58.05 +36:33:43.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 1.327 333411718415722752 039.99149675064 +36.56226419982 13.8411 13.4230 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.327#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151751_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151751_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 02:39:50.25 +35:25:16.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 2.317 141043947159044480 039.95876408671 +35.42084195141 14.0507 13.5390 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.317#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151759_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151759_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 02:42:10.81 +42:23:35.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151766_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151766_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 03:16:03.11 +35:03:57.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.05, MAG_FAINT_SEARCH_LIMIT=15.03)GAIADR2_OUTPUT=# 4.268 138010050980410496 049.01401730548 +35.06678121470 14.4853 13.8783 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.268#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151775_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151775_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 02:55:19.22 +43:08:01.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151778_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151778_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 03:21:05.90 +42:51:11.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151786_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151786_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 02:41:16.23 +37:32:31.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 4.477 333524968113212672 040.31607059079 +37.54180630225 14.1985 13.4893 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.477#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151804_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151804_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 03:09:41.38 +40:56:29.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 0.934 239191509014945408 047.42246281465 +40.94138190072 14.2949 13.8341 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.934#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151815_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151815_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 03:22:11.31 +34:11:18.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151821_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151821_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 02:44:56.37 +33:26:12.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151823_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151823_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 02:36:37.77 +41:46:19.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151825_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151825_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 03:29:26.33 +36:00:28.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.35, MAG_FAINT_SEARCH_LIMIT=15.33)GAIADR2_OUTPUT=# 1.342 222048370390969984 052.35980610604 +36.00758014214 14.4852 13.8169 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.342#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151831_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151831_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 03:28:17.26 +33:29:17.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151837_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151837_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 02:53:15.12 +39:44:06.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151850_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151850_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 03:13:46.62 +38:33:01.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151865_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 151865_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 03:16:37.10 +40:55:49.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.45, MAG_FAINT_SEARCH_LIMIT=15.43)GAIADR2_OUTPUT=# 2.586 239288197319194752 049.15370036164 +40.93054445776 14.5766 13.9940 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.586#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 93945_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 93945_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 03:14:39.61 +33:18:08.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 96112_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
Preparing report for the candidate 96112_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117547_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 117547_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 03:30:03.08 +35:40:16.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11236_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 11236_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks
**** FOUND 02:59:56.34 +42:37:13.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 108950_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148
The candidate 108950_fd_Per-04-Q1b1x1_2026-02-10_22-40-19_20.00sec_-14.90C_LIGHT_0148 did not pass the final checks