This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj
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!
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,2461093.7263,13.81,0.05,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 20260222.2263 13.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:46:04.51 +41:18:51.6 ;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_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20_00sec_-15_00C_LIGHT_0594_fits__*pix.png resample_wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20_00sec_-15_00C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20_00sec_-15_00C_LIGHT_0594_fits__*pix.png resample_wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20_00sec_-15_00C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20_00sec_-15_00C_LIGHT_0594_fits__*pix.png resample_wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20_00sec_-15_00C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20_00sec_-15_00C_LIGHT_0594_fits__*pix.png resample_wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20_00sec_-15_00C_LIGHT_0213_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
HAT-135-0002759,2461093.7263,13.56,0.05,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
HAT-135-0002759 20260222.2263 13.56CV 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/Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:01:00.36 +44:53:24.1 ;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_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20_00sec_-15_00C_LIGHT_0594_fits__*pix.png resample_wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20_00sec_-15_00C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20_00sec_-15_00C_LIGHT_0594_fits__*pix.png resample_wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20_00sec_-15_00C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20_00sec_-15_00C_LIGHT_0594_fits__*pix.png resample_wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20_00sec_-15_00C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20_00sec_-15_00C_LIGHT_0594_fits__*pix.png resample_wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20_00sec_-15_00C_LIGHT_0213_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2263* 08 40 49.40 +50 08 08.8 12.8 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
X UMa,2461093.7263,12.78,0.05,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
X UMa 20260222.2263 12.78CV 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/Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:40:49.40 +50:08:08.8 ;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_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20_00sec_-15_00C_LIGHT_0594_fits__*pix.png resample_wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20_00sec_-15_00C_LIGHT_0214_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20_00sec_-15_00C_LIGHT_0594_fits__*pix.png resample_wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20_00sec_-15_00C_LIGHT_0213_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20_00sec_-15_00C_LIGHT_0594_fits__*pix.png resample_wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20_00sec_-15_00C_LIGHT_0214_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20_00sec_-15_00C_LIGHT_0594_fits__*pix.png resample_wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20_00sec_-15_00C_LIGHT_0213_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: 2461032.95850285 23.12.2025 11:00:04.646 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits
First image: 2461032.95850285 23.12.2025 11:00:04.646 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits
Last image: 2461093.72660829 22.02.2026 05:26:08.956 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.42
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): 11432
Objects passed selection criteria: 11431
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 11164
Average stars matched: 10883.5 (97.4875 %)
Memory usage VmPeak: 116656 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Feb 22 05:27:37 CST 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.95850285 23.12.2025 11:00:04.646 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits
First image: 2461032.95850285 23.12.2025 11:00:04.646 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits
Last image: 2461093.72660829 22.02.2026 05:26:08.956 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 181
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.18
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: 30 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): 66139
Objects passed selection criteria: 65955
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 64200.2
Average stars matched: 62049.5 (96.6499 %)
Memory usage VmPeak: 1923024 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Feb 22 05:29:24 CST 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits
SExtractor catalog cache: saved Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits.cat to cache
SExtractor catalog cache: saved Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.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/Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.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: 2461093.72607774
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_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits exists and is non-empty
Saving wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits to local_wcs_cache/
'wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits' -> 'local_wcs_cache/wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits'
wcs_Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits exists and is non-empty
Saving wcs_Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits to local_wcs_cache/
'wcs_Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits' -> 'local_wcs_cache/wcs_Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits'
wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits exists and is non-empty
Saving wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits to local_wcs_cache/
'wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits' -> 'local_wcs_cache/wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits'
wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits exists and is non-empty
Saving wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits to local_wcs_cache/
'wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits' -> 'local_wcs_cache/wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.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 08:24:00.794 +45:59:46.50
Second-epoch image center 08:24:01.456 +45:59:35.71
Angular distance between the image centers 0.00 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:24:00.794 +45:59:46.50
Second-epoch image center 08:24:02.295 +45:59:06.31
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 08:24:01.456 +45:59:35.71
Second-epoch second image center 08:24:02.295 +45:59:06.31
Angular distance between the image centers 0.00852 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/Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits &> /tmp/tmp.UXA25JAstR
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits &> /tmp/tmp.NrfdqqKUhj
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits &> /tmp/tmp.hFen7RO3nl
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits &> /tmp/tmp.xN2hsGFNiA
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits
Calibrating the magnitude scale
Found non-empty wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.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_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits and wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.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_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits and wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits.cat
Found non-empty wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits and wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits.cat
The reference image (wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits) and catalog (wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits.cat) found
'wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.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 4746 out of 11245 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.959986
a=0.000000 b=1.000000 c=22.959986
From vast_summary.log: estimated ref. image limiting mag.: -7.42
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
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits
2.1 pix Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits
2.3 pix fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits
2.2 pix fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits
Limiting magnitude estimates:
15.5 mag. Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits
15.5 mag. Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits
15.5 mag. fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits
15.5 mag. fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits
All-image limiting magnitude estimate: 15.5 (SNR ) 12.4 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.UXA25JAstR (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits' -> 'wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits
WCS_IMAGE_NAME=wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits
WCS-calibrated image found: wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits
Checking if the catalog wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits.cat corresponding to the image wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits alredy exist and is non-empty...
Catalog wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits.cat corresponding to the image wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits
WCS catalog name: wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=792, passed=11245
Got 11245 stars (including 10435 good ones) from the SExtractor catalog wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits.cat
util/solve_plate_with_UCAC5 got 11245 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.32"
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits -region wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.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.NrfdqqKUhj (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits' -> 'wcs_Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits
WCS_IMAGE_NAME=wcs_Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits
WCS-calibrated image found: wcs_Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits
Checking if the catalog wcs_Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits.cat corresponding to the image wcs_Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits alredy exist and is non-empty...
Catalog wcs_Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits.cat corresponding to the image wcs_Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits
WCS catalog name: wcs_Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=796, passed=11287
Got 11287 stars (including 10475 good ones) from the SExtractor catalog wcs_Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits.cat
util/solve_plate_with_UCAC5 got 11287 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
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 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits -region wcs_Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.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.hFen7RO3nl (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits
WCS-calibrated image found: wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits
Checking if the catalog wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits.cat corresponding to the image wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits.cat corresponding to the image wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits
WCS catalog name: wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=822, passed=11201
Got 11201 stars (including 10361 good ones) from the SExtractor catalog wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits.cat
util/solve_plate_with_UCAC5 got 11201 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.40"
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits -region wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.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.xN2hsGFNiA (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits
WCS-calibrated image found: wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits
Checking if the catalog wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits.cat corresponding to the image wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits.cat corresponding to the image wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits
WCS catalog name: wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=832, passed=11206
Got 11206 stars (including 10355 good ones) from the SExtractor catalog wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits.cat
util/solve_plate_with_UCAC5 got 11206 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 975 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: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
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 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.42"
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits -region wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits'
Saving fully-calibrated image wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits'
Preparing the HTML report for the field Lyn-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20630.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20632.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20622_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214
The candidate 20622_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214 did not pass the final checks
**** FOUND 08:24:24.49 +50:00:50.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20624_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214
The candidate 20624_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214 did not pass the final checks
**** FOUND 08:27:57.23 +45:55:19.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20630_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214
The candidate 20630_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214 did not pass the final checks
**** FOUND 08:45:10.28 +50:09:13.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 1.585 1015445000237826560 131.29244454215 +50.15402963687 12.8036 12.3663 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.585#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20632_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214
The candidate 20632_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214 did not pass the final checks
**** FOUND 08:40:49.42 +50:08:09.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 2.338 1027399234251398144 130.20629849273 +50.13662936605 10.8545 9.5429 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.338#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Lyn-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits
SExtractor catalog cache: saved Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits.cat to cache
SExtractor catalog cache: saved Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits
Creating symlink local_wcs_cache/wcs_Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits
Creating symlink local_wcs_cache/wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits
Creating symlink local_wcs_cache/wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.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_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits exists and is non-empty
wcs_Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits exists and is non-empty
wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits exists and is non-empty
wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.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 08:24:00.794 +45:59:46.50
Second-epoch image center 08:24:01.456 +45:59:35.71
Angular distance between the image centers 0.00 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:24:00.794 +45:59:46.50
Second-epoch image center 08:24:02.295 +45:59:06.31
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 08:24:01.456 +45:59:35.71
Second-epoch second image center 08:24:02.295 +45:59:06.31
Angular distance between the image centers 0.00852 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/Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits &> /tmp/tmp.JlH3qcIDpA
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits &> /tmp/tmp.EKmXVSF1ax
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits &> /tmp/tmp.0XboTd6eRB
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits &> /tmp/tmp.Qalgi2oXBa
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits
Calibrating the magnitude scale
Found non-empty wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.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_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits and wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.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_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits and wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits.cat
Found non-empty wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits and wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits.cat
The reference image (wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits) and catalog (wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits.cat) found
'wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.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 4751 out of 65324 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.859634
a=0.000000 b=1.000000 c=22.859634
From vast_summary.log: estimated ref. image limiting mag.: -7.18
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.68
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.68
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 27 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits
2.0 pix Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits
2.1 pix fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits
2.1 pix fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits
Limiting magnitude estimates:
15.7 mag. Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits
15.7 mag. Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits
15.6 mag. fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits
15.6 mag. fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits
All-image limiting magnitude estimate: 15.6 (SNR ) 14.9 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.JlH3qcIDpA (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits' -> 'wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits
WCS_IMAGE_NAME=wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits
WCS-calibrated image found: wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits
Checking if the catalog wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits.cat corresponding to the image wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits alredy exist and is non-empty...
Catalog wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits.cat corresponding to the image wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits
WCS catalog name: wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=23, blended=3613, passed=65301
Got 65301 stars (including 61589 good ones) from the SExtractor catalog wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits.cat
util/solve_plate_with_UCAC5 got 65301 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 974 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: 0.34"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits -region wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-04-Q1b1x1_2025-12-23_05-00-04_20.00sec_-15.00C_LIGHT_0594.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.EKmXVSF1ax (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits' -> 'wcs_Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits
WCS_IMAGE_NAME=wcs_Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits
WCS-calibrated image found: wcs_Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits
Checking if the catalog wcs_Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits.cat corresponding to the image wcs_Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits alredy exist and is non-empty...
Catalog wcs_Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits.cat corresponding to the image wcs_Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits
WCS catalog name: wcs_Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=31, blended=3617, passed=64969
Got 64969 stars (including 61235 good ones) from the SExtractor catalog wcs_Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits.cat
util/solve_plate_with_UCAC5 got 64969 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
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 975 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: 0.33"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits -region wcs_Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-04-Q1b1x1_2025-12-23_05-01-02_20.00sec_-15.00C_LIGHT_0595.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.0XboTd6eRB (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits
WCS-calibrated image found: wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits
Checking if the catalog wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits.cat corresponding to the image wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits.cat corresponding to the image wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits
WCS catalog name: wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=41, blended=3973, passed=64090
Got 64090 stars (including 59996 good ones) from the SExtractor catalog wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits.cat
util/solve_plate_with_UCAC5 got 64090 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
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 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.42"
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits -region wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.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.Qalgi2oXBa (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits
WCS-calibrated image found: wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits
Checking if the catalog wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits.cat corresponding to the image wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits.cat corresponding to the image wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits
WCS catalog name: wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=44, blended=3999, passed=64141
Got 64141 stars (including 60025 good ones) from the SExtractor catalog wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits.cat
util/solve_plate_with_UCAC5 got 64141 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 977 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: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.44"
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits -region wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-25-23_20.00sec_-15.00C_LIGHT_0213.fits
Saving fully-calibrated image wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-04-Q1b1x1_232824_TTUQ1b1x1_31949_HiaqYJnj/wcs_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214.fits
Preparing the HTML report for the field Lyn-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out79913.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79916.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79918.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79920.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79924.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79932.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out05506.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46848.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79964.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 9s
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 79913_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214
The candidate 79913_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214 did not pass the final checks
**** FOUND 07:52:10.31 +44:20:21.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)GAIADR2_OUTPUT=# 0.849 926336695271884160 118.04268286135 +44.33946293020 14.3386 13.7610 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.849#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79916_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214
The candidate 79916_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214 did not pass the final checks
**** FOUND 07:46:28.70 +42:37:25.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)GAIADR2_OUTPUT=# 0.732 924279543375755008 116.61933384008 +42.62380953980 14.3799 13.8251 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.732#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79918_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214
The candidate 79918_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214 did not pass the final checks
**** FOUND 07:42:55.29 +44:19:19.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.27, MAG_FAINT_SEARCH_LIMIT=15.25)GAIADR2_OUTPUT=# 1.876 926722726932627584 115.72964827784 +44.32203554946 14.2829 13.7043 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.876#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79920_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214
The candidate 79920_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214 did not pass the final checks
**** FOUND 08:23:52.84 +47:36:01.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 0.943 930481063834171392 125.96989828740 +47.60068928908 13.9825 13.4156 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.943#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79922_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214
The candidate 79922_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214 did not pass the final checks
**** FOUND 07:44:33.37 +44:17:07.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79923_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214
The candidate 79923_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214 did not pass the final checks
**** FOUND 07:48:39.86 +41:39:27.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79924_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214
The candidate 79924_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214 did not pass the final checks
**** FOUND 08:14:21.97 +44:28:43.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 2.445 928229676337070720 123.59102786506 +44.47929408761 13.9905 13.4464 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.445#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79925_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214
The candidate 79925_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214 did not pass the final checks
**** FOUND 08:00:16.30 +43:16:32.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79927_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214
The candidate 79927_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214 did not pass the final checks
**** FOUND 07:59:11.55 +43:21:21.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79928_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214
The candidate 79928_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214 did not pass the final checks
**** FOUND 07:57:54.91 +41:44:53.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79929_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214
The candidate 79929_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214 did not pass the final checks
**** FOUND 08:30:22.89 +49:55:45.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79930_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214
The candidate 79930_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214 did not pass the final checks
**** FOUND 07:40:07.03 +45:00:39.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79931_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214
The candidate 79931_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214 did not pass the final checks
**** FOUND 07:45:22.08 +41:38:12.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79932_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214
The candidate 79932_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214 did not pass the final checks
**** FOUND 08:01:59.24 +46:23:56.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 0.587 932438709927944960 120.49684272049 +46.39924627916 12.2571 11.7210 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.587#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79933_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214
The candidate 79933_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214 did not pass the final checks
**** FOUND 07:48:34.68 +42:51:15.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79940_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214
The candidate 79940_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214 did not pass the final checks
**** FOUND 07:57:04.68 +42:15:08.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79945_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214
The candidate 79945_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214 did not pass the final checks
**** FOUND 07:45:40.45 +47:12:36.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79955_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214
The candidate 79955_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214 did not pass the final checks
**** FOUND 07:54:02.10 +42:14:01.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79960_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214
The candidate 79960_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214 did not pass the final checks
**** FOUND 07:51:15.95 +43:24:22.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79964_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214
Preparing report for the candidate 79964_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214
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Considering the candidate 79971_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214
The candidate 79971_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214 did not pass the final checks
**** FOUND 07:48:56.52 +43:51:00.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79973_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214
The candidate 79973_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214 did not pass the final checks
**** FOUND 07:58:45.26 +43:58:54.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79982_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214
The candidate 79982_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214 did not pass the final checks
**** FOUND 07:46:32.00 +43:05:28.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 07455_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214
The candidate 07455_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214 did not pass the final checks
**** FOUND 08:24:24.52 +50:00:50.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 46848_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214
Preparing report for the candidate 46848_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214
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Considering the candidate 05506_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214
Preparing report for the candidate 05506_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214
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Considering the candidate 55402_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214
The candidate 55402_fd_Lyn-04-Q1b1x1_2026-02-21_23-26-08_20.00sec_-15.00C_LIGHT_0214 did not pass the final checks