This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP
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,2461124.7462,13.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260325.2462 13.77CV 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-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:28:54.24 +36:13:37.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20_00sec_-14_90C_LIGHT_0203_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20_00sec_-15_00C_LIGHT_0017_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20_00sec_-14_90C_LIGHT_0203_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20_00sec_-15_00C_LIGHT_0016_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20_00sec_-14_90C_LIGHT_0203_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20_00sec_-15_00C_LIGHT_0017_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20_00sec_-14_90C_LIGHT_0203_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20_00sec_-15_00C_LIGHT_0016_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,2461124.7462,14.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260325.2462 14.26CV 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-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:45:56.89 +34:12:58.5 ;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-05-Q2b1x1_2026-02-11_23-14-20_20_00sec_-14_90C_LIGHT_0203_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20_00sec_-15_00C_LIGHT_0017_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20_00sec_-14_90C_LIGHT_0203_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20_00sec_-15_00C_LIGHT_0016_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20_00sec_-14_90C_LIGHT_0203_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20_00sec_-15_00C_LIGHT_0017_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20_00sec_-14_90C_LIGHT_0203_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20_00sec_-15_00C_LIGHT_0016_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
NSV 17460,2461124.7462,10.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 17460 20260325.2462 10.93CV 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-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:25:33.71 +37:45:26.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20_00sec_-14_90C_LIGHT_0203_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20_00sec_-15_00C_LIGHT_0017_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20_00sec_-14_90C_LIGHT_0203_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20_00sec_-15_00C_LIGHT_0016_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20_00sec_-14_90C_LIGHT_0203_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20_00sec_-15_00C_LIGHT_0017_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20_00sec_-14_90C_LIGHT_0203_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20_00sec_-15_00C_LIGHT_0016_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: 2461083.71840488 12.02.2026 05:14:20.182 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
First image: 2461083.71840488 12.02.2026 05:14:20.182 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
Last image: 2461124.74651103 25.03.2026 05:54:48.553 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.48
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: 4 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): 12257
Objects passed selection criteria: 12208
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 9218
Average stars matched: 9025.25 (97.909 %)
Memory usage VmPeak: 118848 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Mar 25 01:10:10 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461083.71840488 12.02.2026 05:14:20.182 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
First image: 2461083.71840488 12.02.2026 05:14:20.182 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
Last image: 2461124.74651103 25.03.2026 05:54:48.553 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 49
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.18
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 41 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): 77892
Objects passed selection criteria: 77706
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 61872
Average stars matched: 60098.8 (97.134 %)
Memory usage VmPeak: 2452804 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Mar 25 01:11:48 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits
SExtractor catalog cache: saved Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat to cache
SExtractor catalog cache: saved Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.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-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.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: 2461124.74588515
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-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits exists and is non-empty
Saving wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits to local_wcs_cache/
'wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits' -> 'local_wcs_cache/wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits'
wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits exists and is non-empty
Saving wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits to local_wcs_cache/
'wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits' -> 'local_wcs_cache/wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits'
wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits exists and is non-empty
Saving wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits to local_wcs_cache/
'wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits' -> 'local_wcs_cache/wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits'
wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits exists and is non-empty
Saving wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits to local_wcs_cache/
'wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits' -> 'local_wcs_cache/wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.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 07:38:11.466 +37:59:42.13
Second-epoch image center 07:38:11.081 +38:01:56.18
Angular distance between the image centers 0.04 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 07:38:11.466 +37:59:42.13
Second-epoch image center 07:38:11.572 +38:01:23.05
Angular distance between the image centers 0.03 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 07:38:11.081 +38:01:56.18
Second-epoch second image center 07:38:11.572 +38:01:23.05
Angular distance between the image centers 0.00934 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-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits &> /tmp/tmp.GR2IQpe6bX
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits &> /tmp/tmp.Kvg5hr7xiJ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits &> /tmp/tmp.903kadAplW
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits &> /tmp/tmp.A6TqqSMSoA
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits
Calibrating the magnitude scale
Found non-empty wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.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-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits and wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.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-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits and wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat
Found non-empty wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits and wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat
The reference image (wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits) and catalog (wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat) found
'wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.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 7673 out of 16511 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.914913
a=0.000000 b=1.000000 c=22.914913
From vast_summary.log: estimated ref. image limiting mag.: -7.48
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.43
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.43
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
2.1 pix Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
2.4 pix fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits
2.4 pix fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits
Limiting magnitude estimates:
15.4 mag. Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
15.4 mag. Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
14.2 mag. fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits
14.2 mag. fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 11.3 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.GR2IQpe6bX (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.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-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits' -> 'wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
WCS_IMAGE_NAME=wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
WCS-calibrated image found: wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
Checking if the catalog wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat corresponding to the image wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits alredy exist and is non-empty...
Catalog wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat corresponding to the image wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
WCS catalog name: wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1352, passed=16511
Got 16511 stars (including 15129 good ones) from the SExtractor catalog wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat
util/solve_plate_with_UCAC5 got 16511 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 958 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: 0.33"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits -region wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.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.Kvg5hr7xiJ (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.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-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits' -> 'wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
WCS_IMAGE_NAME=wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
WCS-calibrated image found: wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
Checking if the catalog wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits.cat corresponding to the image wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits alredy exist and is non-empty...
Catalog wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits.cat corresponding to the image wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
WCS catalog name: wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1382, passed=16387
Got 16387 stars (including 14973 good ones) from the SExtractor catalog wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits.cat
util/solve_plate_with_UCAC5 got 16387 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits -region wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.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.903kadAplW (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits
WCS-calibrated image found: wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits
Checking if the catalog wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits.cat corresponding to the image wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits.cat corresponding to the image wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits
WCS catalog name: wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=445, passed=6935
Got 6935 stars (including 6484 good ones) from the SExtractor catalog wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits.cat
util/solve_plate_with_UCAC5 got 6935 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 950 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: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.57"
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 950 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.58"
Estimated accuracy of the plate solution: 0.62"
Excluding outliers - 949 stars left (next iteration limit 1043)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits -region wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.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.A6TqqSMSoA (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits
WCS-calibrated image found: wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits
Checking if the catalog wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits.cat corresponding to the image wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits.cat corresponding to the image wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits
WCS catalog name: wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=448, passed=6811
Got 6811 stars (including 6350 good ones) from the SExtractor catalog wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits.cat
util/solve_plate_with_UCAC5 got 6811 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 950 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: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.57"
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 950 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.58"
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 949 stars left (next iteration limit 1043)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits -region wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.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_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits'
Saving fully-calibrated image wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits'
Saving fully-calibrated image wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits'
Saving fully-calibrated image wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits'
Preparing the HTML report for the field Lyn-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Lyn-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits
SExtractor catalog cache: saved Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat to cache
SExtractor catalog cache: saved Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.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-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
Creating symlink local_wcs_cache/wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
Creating symlink local_wcs_cache/wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits
Creating symlink local_wcs_cache/wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.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-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits exists and is non-empty
wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits exists and is non-empty
wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits exists and is non-empty
wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.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 07:38:11.466 +37:59:42.13
Second-epoch image center 07:38:11.081 +38:01:56.18
Angular distance between the image centers 0.04 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 07:38:11.466 +37:59:42.13
Second-epoch image center 07:38:11.572 +38:01:23.05
Angular distance between the image centers 0.03 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 07:38:11.081 +38:01:56.18
Second-epoch second image center 07:38:11.572 +38:01:23.05
Angular distance between the image centers 0.00934 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-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits &> /tmp/tmp.FGNgl2Fbzy
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits &> /tmp/tmp.RwnjJO5b53
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits &> /tmp/tmp.aaxBWFOQ3d
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits &> /tmp/tmp.1EQFt6vex8
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits
Calibrating the magnitude scale
Found non-empty wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.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-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits and wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.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-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits and wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat
Found non-empty wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits and wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat
The reference image (wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits) and catalog (wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat) found
'wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.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 7750 out of 100593 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.795616
a=0.000000 b=1.000000 c=22.795616
From vast_summary.log: estimated ref. image limiting mag.: -7.18
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
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 39 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
1.9 pix Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
2.2 pix fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits
2.2 pix fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits
Limiting magnitude estimates:
15.6 mag. Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
15.6 mag. Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
14.4 mag. fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits
14.4 mag. fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 13.9 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.FGNgl2Fbzy (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.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-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits' -> 'wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
WCS_IMAGE_NAME=wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
WCS-calibrated image found: wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
Checking if the catalog wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat corresponding to the image wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits alredy exist and is non-empty...
Catalog wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat corresponding to the image wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
WCS catalog name: wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=28, blended=7850, passed=100565
Got 100565 stars (including 92523 good ones) from the SExtractor catalog wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat
util/solve_plate_with_UCAC5 got 100565 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.36"
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits -region wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.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.RwnjJO5b53 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.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-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits' -> 'wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
WCS_IMAGE_NAME=wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
WCS-calibrated image found: wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
Checking if the catalog wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits.cat corresponding to the image wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits alredy exist and is non-empty...
Catalog wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits.cat corresponding to the image wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
WCS catalog name: wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=35, blended=7890, passed=100818
Got 100818 stars (including 92732 good ones) from the SExtractor catalog wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits.cat
util/solve_plate_with_UCAC5 got 100818 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 950 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: 0.40"
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 950 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.39"
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 950 stars left (next iteration limit 1045)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits -region wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.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.aaxBWFOQ3d (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits
WCS-calibrated image found: wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits
Checking if the catalog wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits.cat corresponding to the image wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits.cat corresponding to the image wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits
WCS catalog name: wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=2193, passed=46081
Got 46081 stars (including 43832 good ones) from the SExtractor catalog wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits.cat
util/solve_plate_with_UCAC5 got 46081 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 952 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: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.53"
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 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.53"
Estimated accuracy of the plate solution: 0.59"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits -region wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.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.1EQFt6vex8 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits
WCS-calibrated image found: wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits
Checking if the catalog wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits.cat corresponding to the image wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits.cat corresponding to the image wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits
WCS catalog name: wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=2236, passed=45023
Got 45023 stars (including 42740 good ones) from the SExtractor catalog wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits.cat
util/solve_plate_with_UCAC5 got 45023 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 952 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: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.55"
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 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.55"
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits -region wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.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_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
Saving fully-calibrated image wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
Saving fully-calibrated image wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-53-54_20.00sec_-15.00C_LIGHT_0016.fits
Saving fully-calibrated image wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Lyn-05-Q2b1x1_010752_TTUQ2b1x1_13021_9kao7HlP/wcs_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017.fits
Preparing the HTML report for the field Lyn-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out117183.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out117189.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out117193.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out117195.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out117196.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out117197.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out117295.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out117360.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out117375.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out117389.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out117398.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out117399.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out117415.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out117426.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out117428.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out117431.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out117433.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out117448.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out117454.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out117456.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out117467.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out117469.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out117471.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out117478.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out117492.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out117549.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out117570.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out117586.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out15044.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out117521.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out117581.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51065.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 117183_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017
The candidate 117183_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017 did not pass the final checks
**** FOUND 07:33:48.47 +36:54:52.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 1.566 898648514286882816 113.45203978359 +36.91509666463 13.8470 13.2461 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.566#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117189_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017
The candidate 117189_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017 did not pass the final checks
**** FOUND 07:08:59.71 +37:45:47.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 2.486 946220057390596608 107.24936300979 +37.76374451626 13.5427 13.0646 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.486#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117193_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017
The candidate 117193_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017 did not pass the final checks
**** FOUND 07:42:49.50 +35:10:28.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 4.119 894452129377099520 115.70486578888 +35.17433024124 13.9860 13.3560 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.119#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117195_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017
The candidate 117195_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017 did not pass the final checks
**** FOUND 07:21:27.00 +40:48:33.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 2.664 948285554406330496 110.36156455552 +40.80903439478 12.6577 12.0034 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.664#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117196_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017
The candidate 117196_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017 did not pass the final checks
**** FOUND 07:48:55.70 +36:42:59.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 1.293 919034735472746880 117.23170614311 +36.71663841966 12.4054 11.9294 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.293#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117197_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017
The candidate 117197_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017 did not pass the final checks
**** FOUND 08:06:31.22 +35:57:05.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 1.086 906181371527959296 121.62977998960 +35.95181420242 11.9705 11.5096 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.086#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 117245_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017
The candidate 117245_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017 did not pass the final checks
**** FOUND 08:01:58.10 +34:06:22.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117281_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017
The candidate 117281_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017 did not pass the final checks
**** FOUND 07:49:42.05 +38:02:01.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117295_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017
The candidate 117295_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017 did not pass the final checks
**** FOUND 07:40:24.07 +39:48:17.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 0.588 923366021012583680 115.10029215849 +39.80496884373 12.5778 12.1407 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.588#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 117296_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017
The candidate 117296_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017 did not pass the final checks
**** FOUND 07:21:59.27 +36:47:29.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 117360_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017
The candidate 117360_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017 did not pass the final checks
**** FOUND 07:40:32.55 +39:48:05.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.00, MAG_FAINT_SEARCH_LIMIT=13.98)GAIADR2_OUTPUT=# 0.537 923363134794557696 115.13560752081 +39.80178739724 13.1638 12.7194 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.537#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 117367_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017
The candidate 117367_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017 did not pass the final checks
**** FOUND 07:42:50.80 +34:00:37.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 117375_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017
The candidate 117375_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017 did not pass the final checks
**** FOUND 07:33:16.72 +37:10:46.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 1.101 898666965466371840 113.31942822917 +37.17968410198 12.9172 12.2005 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.101#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 117389_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017
The candidate 117389_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017 did not pass the final checks
**** FOUND 07:17:35.81 +40:55:56.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 2.837 948507690114493312 109.39817583515 +40.93250018618 12.8422 12.0974 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.837#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 117394_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017
The candidate 117394_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017 did not pass the final checks
**** FOUND 08:07:53.17 +38:35:53.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117398_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017
The candidate 117398_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017 did not pass the final checks
**** FOUND 07:28:24.89 +37:23:33.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 1.810 898816640783435776 112.10406171757 +37.39224957736 13.3045 12.8715 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.810#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 117399_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017
The candidate 117399_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017 did not pass the final checks
**** FOUND 07:38:12.18 +38:17:16.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 1.583 899192428948922624 114.55051250439 +38.28831501662 13.4657 12.7179 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.583#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 117415_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017
The candidate 117415_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017 did not pass the final checks
**** FOUND 07:36:35.32 +35:26:09.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 0.285 895306209393271936 114.14726326335 +35.43609158216 13.3870 13.4491 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.285#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 117426_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017
The candidate 117426_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017 did not pass the final checks
**** FOUND 07:11:01.18 +37:16:45.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 1.862 945957686427806720 107.75454275739 +37.27877124072 13.1463 12.7110 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.862#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 117428_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017
The candidate 117428_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017 did not pass the final checks
**** FOUND 07:55:10.24 +41:56:45.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 1.772 922500808439917184 118.79323762064 +41.94563987437 13.4751 12.9905 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.772#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 117431_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017
The candidate 117431_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017 did not pass the final checks
**** FOUND 07:23:47.10 +34:14:24.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 0.239 896404724589021056 110.94632169850 +34.24005768735 13.3615 12.9213 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.239#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 117433_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017
The candidate 117433_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017 did not pass the final checks
**** FOUND 07:32:12.73 +36:09:03.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 0.835 895502571001614976 113.05279795040 +36.15082150136 13.2965 12.8586 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.835#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 117448_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017
The candidate 117448_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017 did not pass the final checks
**** FOUND 07:32:37.99 +36:18:11.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 1.500 895511543189782912 113.15824706600 +36.30355400896 13.5844 13.1538 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.500#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 117454_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017
The candidate 117454_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017 did not pass the final checks
**** FOUND 07:18:17.98 +36:59:55.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 0.693 898042855179894912 109.57512916473 +36.99886868458 13.6998 13.1913 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.693#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 117456_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017
The candidate 117456_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017 did not pass the final checks
**** FOUND 07:55:34.33 +35:58:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 3.269 906743844741445632 118.89239763549 +35.98052154056 13.6702 13.2140 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.269#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 117467_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017
The candidate 117467_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017 did not pass the final checks
**** FOUND 08:03:35.53 +36:22:55.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 1.746 906994292874236544 120.89778801373 +36.38243990038 13.7160 13.0416 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.746#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 117469_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017
The candidate 117469_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017 did not pass the final checks
**** FOUND 08:06:10.92 +34:40:32.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 2.176 905494730812530816 121.54610114047 +34.67590343364 13.5187 12.9172 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.176#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 117471_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017
The candidate 117471_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017 did not pass the final checks
**** FOUND 07:23:32.68 +38:09:31.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 0.593 899717514467715456 110.88598727230 +38.15869601085 13.5707 13.0437 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.593#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 117478_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017
The candidate 117478_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017 did not pass the final checks
**** FOUND 07:25:21.37 +36:23:57.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 1.595 897256949179628160 111.33914568328 +36.39962957972 14.1248 13.4678 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.595#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 117492_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017
The candidate 117492_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017 did not pass the final checks
**** FOUND 07:27:09.53 +37:38:54.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 0.801 898883195596665216 111.78960126077 +37.64859456578 13.9858 13.4374 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.801#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 117521_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017
Preparing report for the candidate 117521_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017
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Considering the candidate 117541_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017
The candidate 117541_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017 did not pass the final checks
**** FOUND 07:45:01.86 +40:43:23.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117549_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017
The candidate 117549_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017 did not pass the final checks
**** FOUND 07:50:04.99 +39:25:16.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 0.905 920515983793749248 117.52064796988 +39.42158675870 14.1670 13.6361 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.905#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 117570_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017
The candidate 117570_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017 did not pass the final checks
**** FOUND 07:49:54.36 +39:34:01.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 3.155 920705649549621120 117.47537208196 +39.56730390486 14.3177 13.7800 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.155#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 117581_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017
Preparing report for the candidate 117581_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017
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Considering the candidate 117586_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017
The candidate 117586_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017 did not pass the final checks
**** FOUND 07:56:38.07 +36:53:52.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.28, MAG_FAINT_SEARCH_LIMIT=15.26)GAIADR2_OUTPUT=# 2.519 918911590170434688 119.15778575843 +36.89814272919 14.3978 13.9474 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.519#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 15044_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017
The candidate 15044_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017 did not pass the final checks
**** FOUND 07:54:02.87 +41:19:25.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)
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Considering the candidate 51065_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017
Preparing report for the candidate 51065_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017
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Considering the candidate 42699_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017
The candidate 42699_fd_Lyn-05-Q2b1x1_2026-03-25_00-54-48_20.00sec_-15.00C_LIGHT_0017 did not pass the final checks