This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk
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,2461093.7219,13.59,0.05,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 20260222.2219 13.59CV 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-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:03:44.30 +36:40:47.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20_00sec_-14_90C_LIGHT_0630_fits__*pix.png resample_wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20_00sec_-14_90C_LIGHT_0208_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20_00sec_-14_90C_LIGHT_0630_fits__*pix.png resample_wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20_00sec_-15_00C_LIGHT_0207_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20_00sec_-14_90C_LIGHT_0630_fits__*pix.png resample_wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20_00sec_-14_90C_LIGHT_0630_fits__*pix.png resample_wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20_00sec_-15_00C_LIGHT_0207_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461093.7219,13.78,0.05,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
VARIABLE_NAME 20260222.2219 13.78CV 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-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:46:04.67 +41:18:52.5 ;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-06-Q1b1x1_2025-12-23_05-32-24_20_00sec_-14_90C_LIGHT_0630_fits__*pix.png resample_wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20_00sec_-14_90C_LIGHT_0208_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20_00sec_-14_90C_LIGHT_0630_fits__*pix.png resample_wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20_00sec_-15_00C_LIGHT_0207_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20_00sec_-14_90C_LIGHT_0630_fits__*pix.png resample_wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20_00sec_-14_90C_LIGHT_0630_fits__*pix.png resample_wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20_00sec_-15_00C_LIGHT_0207_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461093.7219,14.28,0.05,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 20260222.2219 14.28CV 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-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:14:36.29 +42:30:21.2 ;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-06-Q1b1x1_2025-12-23_05-32-24_20_00sec_-14_90C_LIGHT_0630_fits__*pix.png resample_wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20_00sec_-14_90C_LIGHT_0208_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20_00sec_-14_90C_LIGHT_0630_fits__*pix.png resample_wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20_00sec_-15_00C_LIGHT_0207_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20_00sec_-14_90C_LIGHT_0630_fits__*pix.png resample_wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20_00sec_-14_90C_LIGHT_0208_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20_00sec_-14_90C_LIGHT_0630_fits__*pix.png resample_wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20_00sec_-15_00C_LIGHT_0207_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: 2461032.98095582 23.12.2025 11:32:24.583 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
First image: 2461032.98095582 23.12.2025 11:32:24.583 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
Last image: 2461093.72216225 22.02.2026 05:19:44.818 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 7
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.45
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: 10 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): 11047
Objects passed selection criteria: 11030
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 10310
Average stars matched: 9916.75 (96.1857 %)
Memory usage VmPeak: 116036 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 02:52:16 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: 2461032.98095582 23.12.2025 11:32:24.583 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
First image: 2461032.98095582 23.12.2025 11:32:24.583 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
Last image: 2461093.72216225 22.02.2026 05:19:44.818 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 236
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.22
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: 85 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): 61331
Objects passed selection criteria: 61162
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 57696
Average stars matched: 54934.2 (95.2133 %)
Memory usage VmPeak: 156908 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 02:55:51 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-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
SExtractor catalog cache: saved Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits.cat to cache
SExtractor catalog cache: saved Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.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-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.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: 2461093.72163340
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-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits exists and is non-empty
Saving wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits to local_wcs_cache/
'wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits' -> 'local_wcs_cache/wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits'
wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits exists and is non-empty
Saving wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits to local_wcs_cache/
'wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits' -> 'local_wcs_cache/wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits'
wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits exists and is non-empty
Saving wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits to local_wcs_cache/
'wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits' -> 'local_wcs_cache/wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits'
wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits exists and is non-empty
Saving wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits to local_wcs_cache/
'wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits' -> 'local_wcs_cache/wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.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 08:43:38.316 +37:59:58.50
Second-epoch image center 08:43:38.069 +38:00:02.88
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 08:43:38.316 +37:59:58.50
Second-epoch image center 08:43:35.737 +38:00:43.05
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 08:43:38.069 +38:00:02.88
Second-epoch second image center 08:43:35.737 +38:00:43.05
Angular distance between the image centers 0.01353 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-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits &> /tmp/tmp.PvvPgijw0g
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits &> /tmp/tmp.Ajq0pRQP4y
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits &> /tmp/tmp.8QXUlRWQnt
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits &> /tmp/tmp.u2Isd2i38z
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
Calibrating the magnitude scale
Found non-empty wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.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-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits and wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.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-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits and wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits.cat
Found non-empty wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits and wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits.cat
The reference image (wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits) and catalog (wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits.cat) found
'wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.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 5313 out of 10418 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.940273
a=0.000000 b=1.000000 c=22.940273
From vast_summary.log: estimated ref. image limiting mag.: -7.45
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.49
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.49
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 7 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
2.1 pix Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits
2.1 pix fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
2.1 pix fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
Limiting magnitude estimates:
15.5 mag. Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
15.5 mag. Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits
15.4 mag. fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
15.4 mag. fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
All-image limiting magnitude estimate: 15.4 (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.PvvPgijw0g (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-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.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-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits' -> 'wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
WCS_IMAGE_NAME=wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
WCS-calibrated image found: wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
Checking if the catalog wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits.cat corresponding to the image wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits alredy exist and is non-empty...
Catalog wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits.cat corresponding to the image wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
WCS catalog name: wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=693, passed=10418
Got 10418 stars (including 9715 good ones) from the SExtractor catalog wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits.cat
util/solve_plate_with_UCAC5 got 10418 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 976 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: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
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 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.29"
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits -region wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.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.Ajq0pRQP4y (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-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.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-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits' -> 'wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits
WCS_IMAGE_NAME=wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits
WCS-calibrated image found: wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits
Checking if the catalog wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits.cat corresponding to the image wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits alredy exist and is non-empty...
Catalog wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits.cat corresponding to the image wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits
WCS catalog name: wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=705, passed=10485
Got 10485 stars (including 9770 good ones) from the SExtractor catalog wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits.cat
util/solve_plate_with_UCAC5 got 10485 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 976 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: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
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 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.29"
Estimated accuracy of the plate solution: 0.27"
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-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits -region wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.8QXUlRWQnt (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-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.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-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
WCS-calibrated image found: wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
Checking if the catalog wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits.cat corresponding to the image wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits.cat corresponding to the image wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.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-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
WCS catalog name: wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=776, passed=10305
Got 10305 stars (including 9518 good ones) from the SExtractor catalog wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits.cat
util/solve_plate_with_UCAC5 got 10305 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 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
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 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.36"
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 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_fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits -region wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.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.u2Isd2i38z (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-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.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-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
WCS-calibrated image found: wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
Checking if the catalog wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits.cat corresponding to the image wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits.cat corresponding to the image wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.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-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
WCS catalog name: wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=801, passed=10234
Got 10234 stars (including 9419 good ones) from the SExtractor catalog wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits.cat
util/solve_plate_with_UCAC5 got 10234 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 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: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
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: 0.40"
Estimated accuracy of the plate solution: 0.40"
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_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits -region wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.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-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits'
Saving fully-calibrated image wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits'
Preparing the HTML report for the field Lyn-06-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20913_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
The candidate 20913_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208 did not pass the final checks
**** FOUND 09:06:05.86 +35:36:26.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20918_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
The candidate 20918_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208 did not pass the final checks
**** FOUND 09:11:30.32 +40:08:09.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20928_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
The candidate 20928_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208 did not pass the final checks
**** FOUND 08:39:12.70 +37:45:53.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20937_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
The candidate 20937_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208 did not pass the final checks
**** FOUND 08:50:14.60 +38:23:48.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20940_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
The candidate 20940_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208 did not pass the final checks
**** FOUND 08:45:30.66 +38:11:09.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 00780_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
The candidate 00780_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208 did not pass the final checks
**** FOUND 09:08:47.69 +42:09:20.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04725_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
The candidate 04725_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208 did not pass the final checks
**** FOUND 08:28:08.07 +38:20:22.9 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Lyn-06-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-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
SExtractor catalog cache: saved Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits.cat to cache
SExtractor catalog cache: saved Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.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-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
Creating symlink local_wcs_cache/wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits
Creating symlink local_wcs_cache/wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
Creating symlink local_wcs_cache/wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.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-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits exists and is non-empty
wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits exists and is non-empty
wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits exists and is non-empty
wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.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 08:43:38.316 +37:59:58.50
Second-epoch image center 08:43:38.069 +38:00:02.88
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 08:43:38.316 +37:59:58.50
Second-epoch image center 08:43:35.737 +38:00:43.05
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 08:43:38.069 +38:00:02.88
Second-epoch second image center 08:43:35.737 +38:00:43.05
Angular distance between the image centers 0.01353 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-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits &> /tmp/tmp.PrZ8NX889L
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits &> /tmp/tmp.0OIPugLlYO
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits &> /tmp/tmp.R4H5kZNFs3
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits &> /tmp/tmp.h1ybHnvfRN
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
Calibrating the magnitude scale
Found non-empty wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.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-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits and wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.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-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits and wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits.cat
Found non-empty wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits and wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits.cat
The reference image (wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits) and catalog (wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits.cat) found
'wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.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 5344 out of 57791 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.838130
a=0.000000 b=1.000000 c=22.838130
From vast_summary.log: estimated ref. image limiting mag.: -7.22
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.62
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.62
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 44 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
2.0 pix Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits
2.0 pix fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
2.0 pix fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
Limiting magnitude estimates:
15.6 mag. Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
15.6 mag. Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits
15.6 mag. fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
15.6 mag. fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.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.PrZ8NX889L (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-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/util/wcs_image_calibration.sh: line 129: echo: write error: Broken pipe
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits' -> 'wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
WCS_IMAGE_NAME=wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
WCS-calibrated image found: wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
Checking if the catalog wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits.cat corresponding to the image wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits alredy exist and is non-empty...
Catalog wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits.cat corresponding to the image wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits
WCS catalog name: wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=23, blended=3024, passed=57768
Got 57768 stars (including 54668 good ones) from the SExtractor catalog wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits.cat
util/solve_plate_with_UCAC5 got 57768 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: 0.32"
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 977 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: 0.31"
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-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits -region wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-06-Q1b1x1_2025-12-23_05-32-24_20.00sec_-14.90C_LIGHT_0630.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.0OIPugLlYO (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-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.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-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits' -> 'wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits
WCS_IMAGE_NAME=wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits
WCS-calibrated image found: wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits
Checking if the catalog wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits.cat corresponding to the image wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits alredy exist and is non-empty...
Catalog wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits.cat corresponding to the image wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits
WCS catalog name: wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=3079, passed=57501
Got 57501 stars (including 54340 good ones) from the SExtractor catalog wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits.cat
util/solve_plate_with_UCAC5 got 57501 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
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: 0.32"
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 977 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: 0.29"
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-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits -region wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-06-Q1b1x1_2025-12-23_05-33-08_20.00sec_-15.00C_LIGHT_0631.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.R4H5kZNFs3 (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-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.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-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
WCS-calibrated image found: wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
Checking if the catalog wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits.cat corresponding to the image wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits.cat corresponding to the image wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.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-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
WCS catalog name: wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=3518, passed=58317
Got 58317 stars (including 54703 good ones) from the SExtractor catalog wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits.cat
util/solve_plate_with_UCAC5 got 58317 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 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.37"
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 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_fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits -region wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.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.h1ybHnvfRN (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-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.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-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
WCS-calibrated image found: wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
Checking if the catalog wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits.cat corresponding to the image wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits.cat corresponding to the image wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.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-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
WCS catalog name: wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=35, blended=3512, passed=58584
Got 58584 stars (including 54975 good ones) from the SExtractor catalog wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits.cat
util/solve_plate_with_UCAC5 got 58584 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 976 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: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.41"
Estimated accuracy of the plate solution: 0.43"
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_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits -region wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.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-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.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-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-18-59_20.00sec_-15.00C_LIGHT_0207.fits
Saving fully-calibrated image wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.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-06-Q1b1x1_232224_TTUQ1b1x1_9867_TukY8dNk/wcs_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208.fits
Preparing the HTML report for the field Lyn-06-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out03939.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71772.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71783.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71787.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71789.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71790.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71791.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71800.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out73006.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out73044.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out73188.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out72549.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72668.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72994.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 12s
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: 4s
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Considering the candidate 71771_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
The candidate 71771_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208 did not pass the final checks
**** FOUND 08:14:44.38 +32:43:43.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71772_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
The candidate 71772_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208 did not pass the final checks
**** FOUND 08:06:41.01 +41:47:09.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.48, MAG_FAINT_SEARCH_LIMIT=15.46)GAIADR2_OUTPUT=# 1.118 921888895859655296 121.67082261706 +41.78571975158 14.6103 14.0721 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.118#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71776_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
The candidate 71776_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208 did not pass the final checks
**** FOUND 08:13:16.69 +34:33:53.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71777_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
The candidate 71777_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208 did not pass the final checks
**** FOUND 08:06:48.70 +35:24:45.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71781_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
The candidate 71781_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208 did not pass the final checks
**** FOUND 09:16:50.25 +40:37:18.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71783_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
The candidate 71783_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208 did not pass the final checks
**** FOUND 08:16:17.66 +37:16:37.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.19, MAG_FAINT_SEARCH_LIMIT=15.17)
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Considering the candidate 71784_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
The candidate 71784_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208 did not pass the final checks
**** FOUND 08:18:54.89 +37:40:21.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71786_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
The candidate 71786_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208 did not pass the final checks
**** FOUND 09:23:14.42 +41:19:12.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71787_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
The candidate 71787_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208 did not pass the final checks
**** FOUND 09:20:43.30 +41:58:02.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 1.486 815921572947173504 140.18052443201 +41.96698407339 14.2829 13.8023 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.486#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71788_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
The candidate 71788_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208 did not pass the final checks
**** FOUND 09:21:09.41 +42:38:11.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71789_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
The candidate 71789_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208 did not pass the final checks
**** FOUND 08:23:47.44 +36:52:54.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 4.105 904957408927828480 125.94895957280 +36.88140854475 13.8564 13.3505 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.105#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71790_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
The candidate 71790_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208 did not pass the final checks
**** FOUND 08:08:37.87 +33:14:53.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 1.572 902293502709058816 122.15830547948 +33.24835564220 13.9189 13.4835 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.572#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71791_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
The candidate 71791_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208 did not pass the final checks
**** FOUND 08:21:37.50 +35:27:35.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.00, MAG_FAINT_SEARCH_LIMIT=14.98)GAIADR2_OUTPUT=# 1.190 904313438711362176 125.40664930369 +35.45966293890 14.0137 13.4703 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.190#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71792_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
The candidate 71792_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208 did not pass the final checks
**** FOUND 08:11:13.17 +36:33:33.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71794_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
The candidate 71794_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208 did not pass the final checks
**** FOUND 08:26:12.88 +36:38:55.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71795_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
The candidate 71795_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208 did not pass the final checks
**** FOUND 08:07:07.55 +38:21:48.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71797_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
The candidate 71797_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208 did not pass the final checks
**** FOUND 08:16:30.90 +38:59:49.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71800_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
The candidate 71800_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208 did not pass the final checks
**** FOUND 08:27:38.12 +37:17:12.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 2.075 904899787646572800 126.90953181165 +37.28651322200 13.1464 12.6656 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.075#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71831_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
The candidate 71831_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208 did not pass the final checks
**** FOUND 08:27:01.89 +32:46:30.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72238_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
The candidate 72238_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208 did not pass the final checks
**** FOUND 08:08:39.80 +32:40:20.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72389_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
The candidate 72389_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208 did not pass the final checks
**** FOUND 08:20:30.68 +41:53:53.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72413_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
The candidate 72413_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208 did not pass the final checks
**** FOUND 08:08:04.30 +39:21:30.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72485_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
The candidate 72485_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208 did not pass the final checks
**** FOUND 08:14:58.66 +42:18:18.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72549_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
Preparing report for the candidate 72549_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
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Considering the candidate 72668_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
Preparing report for the candidate 72668_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
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Considering the candidate 72691_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
The candidate 72691_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208 did not pass the final checks
**** FOUND 08:24:41.34 +32:46:06.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72742_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
The candidate 72742_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208 did not pass the final checks
**** FOUND 08:02:32.57 +40:51:52.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72795_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
The candidate 72795_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208 did not pass the final checks
**** FOUND 08:25:55.78 +34:08:01.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72846_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
The candidate 72846_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208 did not pass the final checks
**** FOUND 08:22:36.51 +36:38:04.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72854_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
The candidate 72854_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208 did not pass the final checks
**** FOUND 08:03:12.66 +39:30:12.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72994_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
Preparing report for the candidate 72994_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
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Considering the candidate 73006_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
The candidate 73006_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208 did not pass the final checks
**** FOUND 08:23:12.31 +42:46:31.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.17, MAG_FAINT_SEARCH_LIMIT=15.15)GAIADR2_OUTPUT=# 0.934 916203493030781568 125.80162932945 +42.77520097598 14.1910 13.7721 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.934#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 73044_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
The candidate 73044_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208 did not pass the final checks
**** FOUND 08:26:23.04 +40:08:29.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.22, MAG_FAINT_SEARCH_LIMIT=15.20)GAIADR2_OUTPUT=# 1.141 914370126110717184 126.59640765006 +40.14161359623 14.4750 14.0459 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.141#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 73158_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
The candidate 73158_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208 did not pass the final checks
**** FOUND 08:13:43.28 +32:42:58.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 73187_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
The candidate 73187_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208 did not pass the final checks
**** FOUND 08:14:46.92 +32:43:25.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 73188_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
The candidate 73188_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208 did not pass the final checks
**** FOUND 08:26:04.24 +34:53:58.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 2.780 903428538009390720 126.51828797848 +34.90002462466 14.6613 14.1479 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.780#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 73299_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
The candidate 73299_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208 did not pass the final checks
**** FOUND 08:23:50.20 +32:45:59.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 73329_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
The candidate 73329_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208 did not pass the final checks
**** FOUND 08:39:22.40 +41:56:12.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 03975_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
The candidate 03975_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208 did not pass the final checks
**** FOUND 09:08:47.67 +42:09:20.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 69696_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
The candidate 69696_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208 did not pass the final checks
**** FOUND 08:40:41.23 +42:36:33.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 03939_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
The candidate 03939_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208 did not pass the final checks
**** FOUND 09:20:46.75 +41:55:21.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 3.163 815921194990052736 140.19384210836 +41.92327250212 14.0020 13.4610 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.163#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 04523_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
The candidate 04523_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208 did not pass the final checks
**** FOUND 09:16:56.29 +41:54:09.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 02211_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
The candidate 02211_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208 did not pass the final checks
**** FOUND 09:17:15.90 +42:20:49.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 27063_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208
The candidate 27063_fd_Lyn-06-Q1b1x1_2026-02-21_23-19-44_20.00sec_-14.90C_LIGHT_0208 did not pass the final checks