This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE
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 03 22.1830* 04 29 15.07 +39 33 43.7 10.2 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GY Per,2461121.6830,10.18,0.05,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
GY Per 20260322.1830 10.18CV 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-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:29:15.07 +39:33:43.7 ;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-05-Q1b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20_00sec_-15_00C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20_00sec_-15_00C_LIGHT_0004_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!
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,2461121.6830,14.37,0.05,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 20260322.1830 14.37CV 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-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:41:14.43 +35:37:44.3 ;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-05-Q1b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20_00sec_-15_00C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20_00sec_-15_00C_LIGHT_0004_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 03 22.1830* 04 16 01.31 +37 20 27.8 13.4 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
NSVS J0416015+372028,2461121.6830,13.36,0.05,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
NSVS J0416015+372028 20260322.1830 13.36CV 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-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:16:01.31 +37:20:27.8 ;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-05-Q1b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20_00sec_-15_00C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20_00sec_-15_00C_LIGHT_0004_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 03 22.1830* 04 50 00.87 +39 55 58.1 13.0 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
NSVS J0450006+395559,2461121.6830,13.04,0.05,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
NSVS J0450006+395559 20260322.1830 13.04CV 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-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:50:00.87 +39:55:58.1 ;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-05-Q1b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20_00sec_-14_90C_LIGHT_0005_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20_00sec_-15_00C_LIGHT_0004_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20_00sec_-14_90C_LIGHT_0005_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20_00sec_-15_00C_LIGHT_0342_fits__*pix.png resample_wcs_fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20_00sec_-15_00C_LIGHT_0004_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: 2461032.78853589 23.12.2025 06:55:19.501 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
First image: 2461032.78853589 23.12.2025 06:55:19.501 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
Last image: 2461121.68342622 22.03.2026 04:23:58.025 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 7
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.58
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: 6 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): 17570
Objects passed selection criteria: 17558
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 16262.8
Average stars matched: 15945.5 (98.0492 %)
Memory usage VmPeak: 122552 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Mar 21 23:25:50 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.78853589 23.12.2025 06:55:19.501 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
First image: 2461032.78853589 23.12.2025 06:55:19.501 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
Last image: 2461121.68342622 22.03.2026 04:23:58.025 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 53
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.30
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: 46 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): 125060
Objects passed selection criteria: 124869
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 112708
Average stars matched: 109304 (96.9791 %)
Memory usage VmPeak: 1955028 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Mar 21 23:27:55 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/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-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits
SExtractor catalog cache: saved Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.cat to cache
SExtractor catalog cache: saved Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.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-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.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: 2461121.68259481
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-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits exists and is non-empty
Saving wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits to local_wcs_cache/
'wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits' -> 'local_wcs_cache/wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits'
wcs_Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits exists and is non-empty
Saving wcs_Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits to local_wcs_cache/
'wcs_Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits' -> 'local_wcs_cache/wcs_Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits'
wcs_fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits exists and is non-empty
Saving wcs_fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits to local_wcs_cache/
'wcs_fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits' -> 'local_wcs_cache/wcs_fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits'
wcs_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits exists and is non-empty
Saving wcs_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits to local_wcs_cache/
'wcs_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits' -> 'local_wcs_cache/wcs_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 04:21:49.016 +37:59:51.53
Second-epoch image center 04:21:51.821 +37:59:40.56
Angular distance between the image centers 0.01 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 04:21:49.016 +37:59:51.53
Second-epoch image center 04:21:51.599 +37:59:10.89
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 04:21:51.821 +37:59:40.56
Second-epoch second image center 04:21:51.599 +37:59:10.89
Angular distance between the image centers 0.00827 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-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits &> /tmp/tmp.7BcWasJGiu
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits &> /tmp/tmp.ttCWGK7nCA
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits &> /tmp/tmp.NUBHke8FE1
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits &> /tmp/tmp.869BFe1GAF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits
Calibrating the magnitude scale
Found non-empty wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.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-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits and wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.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-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits and wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.cat
Found non-empty wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits and wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.cat
The reference image (wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits) and catalog (wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.cat) found
'wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.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 7129 out of 18677 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.971832
a=0.000000 b=1.000000 c=22.971832
From vast_summary.log: estimated ref. image limiting mag.: -7.58
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.39
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.39
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 6 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
2.1 pix Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
2.4 pix fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits
2.5 pix fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits
Limiting magnitude estimates:
15.4 mag. Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
15.4 mag. Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
14.9 mag. fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits
14.9 mag. fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 12.1 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.7BcWasJGiu (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_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.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-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits' -> 'wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
WCS_IMAGE_NAME=wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
WCS-calibrated image found: wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
Checking if the catalog wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.cat corresponding to the image wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits alredy exist and is non-empty...
Catalog wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.cat corresponding to the image wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
WCS catalog name: wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1808, passed=18677
Got 18677 stars (including 16842 good ones) from the SExtractor catalog wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.cat
util/solve_plate_with_UCAC5 got 18677 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 962 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: 0.38"
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 961 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 - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits -region wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.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.ttCWGK7nCA (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_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.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-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits' -> 'wcs_Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
WCS_IMAGE_NAME=wcs_Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
WCS-calibrated image found: wcs_Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
Checking if the catalog wcs_Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits.cat corresponding to the image wcs_Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits alredy exist and is non-empty...
Catalog wcs_Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits.cat corresponding to the image wcs_Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
WCS catalog name: wcs_Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1789, passed=18684
Got 18684 stars (including 16861 good ones) from the SExtractor catalog wcs_Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits.cat
util/solve_plate_with_UCAC5 got 18684 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 962 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: 0.38"
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 961 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 - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits -region wcs_Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.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.NUBHke8FE1 (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_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.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_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits
WCS_IMAGE_NAME=wcs_fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits
WCS-calibrated image found: wcs_fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits
Checking if the catalog wcs_fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits.cat corresponding to the image wcs_fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits.cat corresponding to the image wcs_fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits
WCS catalog name: wcs_fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=985, passed=14078
Got 14078 stars (including 13076 good ones) from the SExtractor catalog wcs_fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits.cat
util/solve_plate_with_UCAC5 got 14078 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (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: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
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: 0.35"
Estimated accuracy of the plate solution: 0.35"
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_fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits -region wcs_fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.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.869BFe1GAF (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_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.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_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits
WCS_IMAGE_NAME=wcs_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits
WCS-calibrated image found: wcs_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits
Checking if the catalog wcs_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits.cat corresponding to the image wcs_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits.cat corresponding to the image wcs_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits
WCS catalog name: wcs_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1005, passed=14086
Got 14086 stars (including 13060 good ones) from the SExtractor catalog wcs_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits.cat
util/solve_plate_with_UCAC5 got 14086 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (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: 0.36"
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: 0.37"
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_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits -region wcs_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits'
Saving fully-calibrated image wcs_Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/wcs_Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits'
Saving fully-calibrated image wcs_fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/wcs_fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits'
Saving fully-calibrated image wcs_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/wcs_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits'
Preparing the HTML report for the field Per-05-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out08898.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 4s
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 21192_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
The candidate 21192_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 05:00:53.05 +41:47:36.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21206_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
The candidate 21206_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 03:51:16.64 +33:02:10.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21217_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
The candidate 21217_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 04:19:09.16 +40:45:45.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21229_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
The candidate 21229_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 04:29:17.94 +42:33:35.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16341_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
The candidate 16341_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
Rejecting candidate due to large distance (27.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08898_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 08898_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 5s
Prepared the HTML report for the field Per-05-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 ####
04:29:15.07 +39:33:43.7
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-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits
SExtractor catalog cache: saved Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.cat to cache
SExtractor catalog cache: saved Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.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-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
Creating symlink local_wcs_cache/wcs_Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
Creating symlink local_wcs_cache/wcs_fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits
Creating symlink local_wcs_cache/wcs_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.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-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits exists and is non-empty
wcs_Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits exists and is non-empty
wcs_fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits exists and is non-empty
wcs_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 04:21:49.016 +37:59:51.53
Second-epoch image center 04:21:51.821 +37:59:40.56
Angular distance between the image centers 0.01 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 04:21:49.016 +37:59:51.53
Second-epoch image center 04:21:51.599 +37:59:10.89
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 04:21:51.821 +37:59:40.56
Second-epoch second image center 04:21:51.599 +37:59:10.89
Angular distance between the image centers 0.00827 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-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits &> /tmp/tmp.p0QBTisd6r
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits &> /tmp/tmp.ab1n0eZHFr
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits &> /tmp/tmp.zHj52Lc2cp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits &> /tmp/tmp.jIIoxcby2o
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits
Calibrating the magnitude scale
Found non-empty wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.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-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits and wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.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-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits and wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.cat
Found non-empty wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits and wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.cat
The reference image (wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits) and catalog (wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.cat) found
'wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.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 7196 out of 137281 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.837428
a=0.000000 b=1.000000 c=22.837428
From vast_summary.log: estimated ref. image limiting mag.: -7.30
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.54
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.54
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 42 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
2.0 pix Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
2.5 pix fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits
2.5 pix fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits
Limiting magnitude estimates:
15.5 mag. Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
15.5 mag. Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
15.0 mag. fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits
15.0 mag. fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 14.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.p0QBTisd6r (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_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.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-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits' -> 'wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
WCS_IMAGE_NAME=wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
WCS-calibrated image found: wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
Checking if the catalog wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.cat corresponding to the image wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits alredy exist and is non-empty...
Catalog wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.cat corresponding to the image wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
WCS catalog name: wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=23, blended=15371, passed=137258
Got 137258 stars (including 121598 good ones) from the SExtractor catalog wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.cat
util/solve_plate_with_UCAC5 got 137258 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 961 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: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
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 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.38"
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits -region wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.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.ab1n0eZHFr (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_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.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-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits' -> 'wcs_Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
WCS_IMAGE_NAME=wcs_Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
WCS-calibrated image found: wcs_Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
Checking if the catalog wcs_Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits.cat corresponding to the image wcs_Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits alredy exist and is non-empty...
Catalog wcs_Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits.cat corresponding to the image wcs_Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
WCS catalog name: wcs_Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=24, blended=15060, passed=136498
Got 136498 stars (including 121185 good ones) from the SExtractor catalog wcs_Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits.cat
util/solve_plate_with_UCAC5 got 136498 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 965 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: 0.38"
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 965 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: 0.38"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits -region wcs_Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.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.zHj52Lc2cp (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_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.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_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits
WCS_IMAGE_NAME=wcs_fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits
WCS-calibrated image found: wcs_fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits
Checking if the catalog wcs_fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits.cat corresponding to the image wcs_fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits.cat corresponding to the image wcs_fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits
WCS catalog name: wcs_fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=8498, passed=91336
Got 91336 stars (including 82675 good ones) from the SExtractor catalog wcs_fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits.cat
util/solve_plate_with_UCAC5 got 91336 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (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 961 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: 0.35"
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 961 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: 0.36"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits -region wcs_fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.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.jIIoxcby2o (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_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.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_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits
WCS_IMAGE_NAME=wcs_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits
WCS-calibrated image found: wcs_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits
Checking if the catalog wcs_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits.cat corresponding to the image wcs_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits.cat corresponding to the image wcs_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits
WCS catalog name: wcs_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=8269, passed=89203
Got 89203 stars (including 80778 good ones) from the SExtractor catalog wcs_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits.cat
util/solve_plate_with_UCAC5 got 89203 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (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 961 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: 0.35"
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 961 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: 0.36"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits -region wcs_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.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_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/wcs_Per-05-Q1b1x1_2025-12-23_00-55-19_20.00sec_-15.00C_LIGHT_0342.fits
Saving fully-calibrated image wcs_Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.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_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/wcs_Per-05-Q1b1x1_2025-12-23_00-56-00_20.00sec_-15.00C_LIGHT_0343.fits
Saving fully-calibrated image wcs_fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.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_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/wcs_fd_Per-05-Q1b1x1_2026-03-21_23-22-46_20.00sec_-15.00C_LIGHT_0004.fits
Saving fully-calibrated image wcs_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.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_2026-03-21_CI_Per-05-Q1b1x1_232441_TTUQ1b1x1_1740_vk4Ur8ZE/wcs_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005.fits
Preparing the HTML report for the field Per-05-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out159272.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159274.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159293.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159302.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159311.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159313.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160004.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out159915.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52541.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out87160.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 159272_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
The candidate 159272_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 04:46:13.68 +35:30:07.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.72, MAG_FAINT_SEARCH_LIMIT=15.70)
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Considering the candidate 159274_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
The candidate 159274_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 04:15:11.57 +41:04:15.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.53, MAG_FAINT_SEARCH_LIMIT=15.51)
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Considering the candidate 159293_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
The candidate 159293_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 04:17:35.66 +40:53:15.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)GAIADR2_OUTPUT=# 0.150 227931547876730880 064.39855223990 +40.88746544502 14.0414 13.3364 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.150#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 159302_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
The candidate 159302_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 04:31:05.94 +41:00:17.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 4.163 180059120839634560 067.77339837163 +41.00543347935 14.3857 13.7552 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.163#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 159308_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
The candidate 159308_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 04:50:16.78 +41:23:45.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159310_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
The candidate 159310_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 04:21:51.34 +33:46:09.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159311_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
The candidate 159311_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 04:54:41.67 +38:36:49.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.17, MAG_FAINT_SEARCH_LIMIT=15.15)GAIADR2_OUTPUT=# 1.672 199083764376554112 073.67304874364 +38.61375289267 14.0219 13.3215 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.672#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 159313_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
The candidate 159313_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 05:03:13.60 +42:04:33.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)
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Considering the candidate 159326_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
The candidate 159326_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 04:36:10.05 +34:01:40.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159332_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
The candidate 159332_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 03:59:57.41 +42:51:26.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159423_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
The candidate 159423_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 04:09:00.17 +41:28:45.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159431_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
The candidate 159431_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 04:15:31.57 +33:49:31.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159437_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
The candidate 159437_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 04:24:33.20 +34:09:20.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 159493_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
The candidate 159493_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 04:59:26.12 +37:53:17.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 159495_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
The candidate 159495_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 03:44:29.53 +36:26:09.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 159517_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
The candidate 159517_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 03:43:57.82 +38:23:53.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159522_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
The candidate 159522_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 04:32:15.37 +42:36:13.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159530_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
The candidate 159530_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 03:43:40.78 +42:35:50.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159535_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
The candidate 159535_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 04:57:49.29 +39:26:40.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159559_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
The candidate 159559_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 04:24:59.51 +39:52:52.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159582_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
The candidate 159582_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 04:27:10.64 +35:29:46.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159605_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
The candidate 159605_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 04:10:46.35 +38:03:19.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159608_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
The candidate 159608_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 05:00:18.62 +37:12:38.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159615_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
The candidate 159615_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 04:03:09.10 +34:51:12.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159618_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
The candidate 159618_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 04:57:23.02 +41:48:55.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159626_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
The candidate 159626_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 04:32:53.35 +32:52:10.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159627_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
The candidate 159627_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 04:10:49.13 +42:10:40.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159630_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
The candidate 159630_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 04:50:16.71 +38:45:52.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159641_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
The candidate 159641_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 04:23:12.30 +35:29:44.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159726_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
The candidate 159726_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 04:12:08.73 +38:02:39.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159765_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
The candidate 159765_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 04:12:47.98 +39:39:29.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159830_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
The candidate 159830_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 05:01:18.98 +40:39:12.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159915_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 159915_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 159959_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
The candidate 159959_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 04:41:47.64 +37:19:08.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159980_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
The candidate 159980_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 04:21:25.64 +41:52:19.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 160004_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
The candidate 160004_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 04:41:46.65 +37:19:12.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.56, MAG_FAINT_SEARCH_LIMIT=15.54)
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Considering the candidate 87160_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 87160_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 12453_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
The candidate 12453_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 04:29:17.93 +42:33:35.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 94341_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
The candidate 94341_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 03:51:16.67 +33:02:10.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 45725_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
The candidate 45725_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks
**** FOUND 04:19:09.11 +40:45:44.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52541_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
Preparing report for the candidate 52541_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
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Considering the candidate 61976_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005
The candidate 61976_fd_Per-05-Q1b1x1_2026-03-21_23-23-58_20.00sec_-14.90C_LIGHT_0005 did not pass the final checks