This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 26.2899* 15 16 28.49 +16 26 39.6 11.2 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
BF Ser,2461125.7899,11.23,0.05,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
BF Ser 20260326.2899 11.23CV 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/Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits /data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:16:28.49 +16:26:39.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20_00sec_-14_90C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20_00sec_-10_00C_LIGHT_0539_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20_00sec_-14_90C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20_00sec_-10_00C_LIGHT_0538_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20_00sec_-14_90C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20_00sec_-10_00C_LIGHT_0539_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20_00sec_-14_90C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20_00sec_-10_00C_LIGHT_0538_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
CSS_J150956.1+180617,2461125.7899,13.20,0.05,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
CSS_J150956.1+180617 20260326.2899 13.20CV 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/Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits /data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:09:56.16 +18:06:16.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20_00sec_-14_90C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20_00sec_-10_00C_LIGHT_0539_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20_00sec_-14_90C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20_00sec_-10_00C_LIGHT_0538_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20_00sec_-14_90C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20_00sec_-10_00C_LIGHT_0539_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20_00sec_-14_90C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20_00sec_-10_00C_LIGHT_0538_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.2899 2461125.7899 13.62 15:30:06.31 +12:03:40.3
18.78967 49.92862 galactic Ser Second-epoch detections are separated by 1.5" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 15:30:06.31 +12:03:40.3 (user input) | T | P | (position from user input) SpType: K1 (LAMOST DR5) J-Ks=0.467+/-0.034 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 26.2899* 15 30 06.31 +12 03 40.3 13.6 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461125.7899,13.62,0.05,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
target 20260326.2899 13.62CV 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/Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits /data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:30:06.31 +12:03:40.3 ;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_Boo-10-Q2b1x1_2026-02-22_04-23-38_20_00sec_-14_90C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20_00sec_-10_00C_LIGHT_0539_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20_00sec_-14_90C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20_00sec_-10_00C_LIGHT_0538_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20_00sec_-14_90C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20_00sec_-10_00C_LIGHT_0539_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20_00sec_-14_90C_LIGHT_0425_fits__*pix.png resample_wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20_00sec_-10_00C_LIGHT_0538_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: 2461093.93320411 22.02.2026 10:23:38.835 /data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits
First image: 2461093.93320411 22.02.2026 10:23:38.835 /data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits
Last image: 2461125.79015910 26.03.2026 06:57:39.746 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 16
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.68
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: 3 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): 6234
Objects passed selection criteria: 6221
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 5550.75
Average stars matched: 5425.5 (97.7435 %)
Memory usage VmPeak: 112808 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 Thu Mar 26 02:01:00 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: 2461093.93320411 22.02.2026 10:23:38.835 /data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits
First image: 2461093.93320411 22.02.2026 10:23:38.835 /data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits
Last image: 2461125.79015910 26.03.2026 06:57:39.746 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 171
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.39
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: 12 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): 33668
Objects passed selection criteria: 33576
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 31171.5
Average stars matched: 29965 (96.1295 %)
Memory usage VmPeak: 136508 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 Thu Mar 26 02:01:44 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/Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits /data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits
SExtractor catalog cache: saved Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits.cat to cache
SExtractor catalog cache: saved Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.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/Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits /data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.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: 2461125.78964308
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_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits exists and is non-empty
Saving wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits to local_wcs_cache/
'wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits' -> 'local_wcs_cache/wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits'
wcs_Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits exists and is non-empty
Saving wcs_Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits to local_wcs_cache/
'wcs_Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits' -> 'local_wcs_cache/wcs_Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits'
wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits exists and is non-empty
Saving wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits to local_wcs_cache/
'wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits' -> 'local_wcs_cache/wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits'
wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits exists and is non-empty
Saving wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits to local_wcs_cache/
'wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits' -> 'local_wcs_cache/wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits'
The image scale is 5.88"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 15:06:40.111 +13:58:33.68
Second-epoch image center 15:06:48.613 +14:00:05.98
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 15:06:40.111 +13:58:33.68
Second-epoch image center 15:06:47.949 +14:00:09.54
Angular distance between the image centers 0.04 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 15:06:48.613 +14:00:05.98
Second-epoch second image center 15:06:47.949 +14:00:09.54
Angular distance between the image centers 0.00286 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/Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits &> /tmp/tmp.IqPHy50kZY
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits &> /tmp/tmp.ACgyFtpCsS
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits &> /tmp/tmp.jzFy44TUVT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits &> /tmp/tmp.TDcObf1ExU
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits
Calibrating the magnitude scale
Found non-empty wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.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_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits and wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.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_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits and wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits.cat
Found non-empty wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits and wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits.cat
The reference image (wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits) and catalog (wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits.cat) found
'wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.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 3682 out of 7810 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.957583
a=0.000000 b=1.000000 c=22.957583
From vast_summary.log: estimated ref. image limiting mag.: -7.68
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.28
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.28
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 6 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.6 pix Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits
2.5 pix Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits
2.5 pix fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits
2.4 pix fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits
Limiting magnitude estimates:
15.3 mag. Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits
15.3 mag. Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits
15.0 mag. fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits
15.0 mag. fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 12.1 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.IqPHy50kZY (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits' -> 'wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits
WCS_IMAGE_NAME=wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits
WCS-calibrated image found: wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits
Checking if the catalog wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits.cat corresponding to the image wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits alredy exist and is non-empty...
Catalog wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits.cat corresponding to the image wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits
WCS catalog name: wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=467, passed=7810
Got 7810 stars (including 7341 good ones) from the SExtractor catalog wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits.cat
util/solve_plate_with_UCAC5 got 7810 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.44"
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 959 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits -region wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.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.ACgyFtpCsS (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits' -> 'wcs_Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits
WCS_IMAGE_NAME=wcs_Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits
WCS-calibrated image found: wcs_Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits
Checking if the catalog wcs_Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits.cat corresponding to the image wcs_Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits alredy exist and is non-empty...
Catalog wcs_Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits.cat corresponding to the image wcs_Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits
WCS catalog name: wcs_Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=488, passed=7694
Got 7694 stars (including 7199 good ones) from the SExtractor catalog wcs_Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits.cat
util/solve_plate_with_UCAC5 got 7694 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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 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: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
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: 0.45"
Estimated accuracy of the plate solution: 0.45"
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_Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits -region wcs_Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.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.jzFy44TUVT (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_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.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_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits
WCS_IMAGE_NAME=wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits
WCS-calibrated image found: wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits
Checking if the catalog wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits.cat corresponding to the image wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits alredy exist and is non-empty...
Catalog wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits.cat corresponding to the image wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits
WCS catalog name: wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=383, passed=5879
Got 5879 stars (including 5488 good ones) from the SExtractor catalog wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits.cat
util/solve_plate_with_UCAC5 got 5879 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.42"
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits -region wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.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.TDcObf1ExU (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_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.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_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits
WCS_IMAGE_NAME=wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits
WCS-calibrated image found: wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits
Checking if the catalog wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits.cat corresponding to the image wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits alredy exist and is non-empty...
Catalog wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits.cat corresponding to the image wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits
WCS catalog name: wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=398, passed=5873
Got 5873 stars (including 5466 good ones) from the SExtractor catalog wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits.cat
util/solve_plate_with_UCAC5 got 5873 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.43"
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits -region wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.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_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits'
Saving fully-calibrated image wcs_Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/wcs_Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits'
Saving fully-calibrated image wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits'
Saving fully-calibrated image wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits'
Preparing the HTML report for the field Boo-10-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20298.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out05971.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 3s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20298_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 20298_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
**** FOUND 15:23:00.21 +11:22:22.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.54, MAG_FAINT_SEARCH_LIMIT=11.52)GAIADR2_OUTPUT=# 1.039 1169163666467446400 230.75085651104 +11.37317697236 10.5965 10.1584 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.039#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20303_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 20303_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
**** FOUND 15:32:31.94 +18:03:54.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20353_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 20353_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
**** FOUND 15:32:31.73 +17:41:20.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20393_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 20393_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
**** FOUND 15:32:03.74 +18:02:07.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20421_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 20421_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
**** FOUND 15:32:26.39 +17:48:34.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 05971_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
Preparing report for the candidate 05971_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 4s
Prepared the HTML report for the field Boo-10-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 ####
15:16:28.49 +16:26:39.6
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/Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits /data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits
SExtractor catalog cache: saved Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits.cat to cache
SExtractor catalog cache: saved Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits /data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits
Creating symlink local_wcs_cache/wcs_Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits
Creating symlink local_wcs_cache/wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits
Creating symlink local_wcs_cache/wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.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_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits exists and is non-empty
wcs_Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits exists and is non-empty
wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits exists and is non-empty
wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits exists and is non-empty
The image scale is 5.88"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 15:06:40.111 +13:58:33.68
Second-epoch image center 15:06:48.613 +14:00:05.98
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 15:06:40.111 +13:58:33.68
Second-epoch image center 15:06:47.949 +14:00:09.54
Angular distance between the image centers 0.04 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 15:06:48.613 +14:00:05.98
Second-epoch second image center 15:06:47.949 +14:00:09.54
Angular distance between the image centers 0.00286 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/Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits &> /tmp/tmp.HkXStBREws
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits &> /tmp/tmp.NkLKpdKiNE
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits &> /tmp/tmp.KjIoBSOEeM
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits &> /tmp/tmp.MEeCY1tjdk
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits
Calibrating the magnitude scale
Found non-empty wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.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_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits and wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.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_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits and wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits.cat
Found non-empty wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits and wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits.cat
The reference image (wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits) and catalog (wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits.cat) found
'wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.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 3685 out of 38315 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.834385
a=0.000000 b=1.000000 c=22.834385
From vast_summary.log: estimated ref. image limiting mag.: -7.39
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.44
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.44
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 49 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.5 pix Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits
2.4 pix Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits
2.3 pix fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits
2.2 pix fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits
Limiting magnitude estimates:
15.4 mag. Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits
15.5 mag. Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits
15.1 mag. fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits
15.1 mag. fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 14.5 (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.HkXStBREws (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits' -> 'wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits
WCS_IMAGE_NAME=wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits
WCS-calibrated image found: wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits
Checking if the catalog wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits.cat corresponding to the image wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits alredy exist and is non-empty...
Catalog wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits.cat corresponding to the image wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits
WCS catalog name: wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=1972, passed=38305
Got 38305 stars (including 36295 good ones) from the SExtractor catalog wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits.cat
util/solve_plate_with_UCAC5 got 38305 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.43"
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits -region wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.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.NkLKpdKiNE (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits' -> 'wcs_Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits
WCS_IMAGE_NAME=wcs_Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits
WCS-calibrated image found: wcs_Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits
Checking if the catalog wcs_Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits.cat corresponding to the image wcs_Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits alredy exist and is non-empty...
Catalog wcs_Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits.cat corresponding to the image wcs_Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits
WCS catalog name: wcs_Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=2112, passed=39603
Got 39603 stars (including 37440 good ones) from the SExtractor catalog wcs_Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits.cat
util/solve_plate_with_UCAC5 got 39603 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.43"
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits -region wcs_Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.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.KjIoBSOEeM (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_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.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_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits
WCS_IMAGE_NAME=wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits
WCS-calibrated image found: wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits
Checking if the catalog wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits.cat corresponding to the image wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits alredy exist and is non-empty...
Catalog wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits.cat corresponding to the image wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits
WCS catalog name: wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=1329, passed=32608
Got 32608 stars (including 31249 good ones) from the SExtractor catalog wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits.cat
util/solve_plate_with_UCAC5 got 32608 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.44"
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits -region wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.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.MEeCY1tjdk (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_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.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_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits
WCS_IMAGE_NAME=wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits
WCS-calibrated image found: wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits
Checking if the catalog wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits.cat corresponding to the image wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits alredy exist and is non-empty...
Catalog wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits.cat corresponding to the image wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits
WCS catalog name: wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=1382, passed=33231
Got 33231 stars (including 31812 good ones) from the SExtractor catalog wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits.cat
util/solve_plate_with_UCAC5 got 33231 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.43"
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits -region wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.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_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.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_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/wcs_Boo-10-Q2b1x1_2026-02-22_04-23-38_20.00sec_-14.90C_LIGHT_0425.fits
Saving fully-calibrated image wcs_Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.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_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/wcs_Boo-10-Q2b1x1_2026-02-22_04-24-26_20.00sec_-15.00C_LIGHT_0426.fits
Saving fully-calibrated image wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.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_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-56-55_20.00sec_-10.00C_LIGHT_0538.fits
Saving fully-calibrated image wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.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_2026-03-26_CI_Boo-10-Q2b1x1_015848_TTUQ2b1x1_31571_sFsZRPqz/wcs_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539.fits
Preparing the HTML report for the field Boo-10-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out53081.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53082.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53083.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53087.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53089.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53093.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53099.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53466.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53691.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53774.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53805.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53836.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53938.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53978.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54019.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54083.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54153.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54193.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54273.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54275.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54303.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54317.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out14623.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28572.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 14s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 53081_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 53081_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
**** FOUND 15:13:43.14 +14:47:04.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.52, MAG_FAINT_SEARCH_LIMIT=15.50)GAIADR2_OUTPUT=# 2.451 1183165186837030016 228.42995358770 +14.78387614679 14.6888 14.1012 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.451#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53082_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 53082_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
**** FOUND 15:29:15.02 +16:16:02.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.35, MAG_FAINT_SEARCH_LIMIT=15.33)GAIADR2_OUTPUT=# 0.643 1207570913295516416 232.31248720066 +16.26712498528 14.0273 13.3283 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.643#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53083_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 53083_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
**** FOUND 15:32:02.93 +14:44:35.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)GAIADR2_OUTPUT=# 0.639 1194837297335572992 233.01233334789 +14.74318547393 14.5142 14.0032 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.639#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53087_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 53087_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
**** FOUND 14:42:56.70 +09:49:50.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.25, MAG_FAINT_SEARCH_LIMIT=15.23)GAIADR2_OUTPUT=# 1.675 1174743928495851392 220.73660287639 +09.83092021083 14.3521 13.7874 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.675#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53088_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 53088_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
**** FOUND 15:17:18.77 +18:02:08.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53089_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 53089_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
**** FOUND 15:25:48.51 +17:32:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 0.888 1208042397625279360 231.45202306780 +17.54975456854 14.2029 13.4757 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.888#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53093_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 53093_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
**** FOUND 15:29:57.05 +16:47:32.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 0.363 1207741784274248576 232.48775457804 +16.79238167758 13.9306 13.2826 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.363#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53094_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 53094_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
**** FOUND 15:30:14.19 +18:01:36.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53096_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 53096_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
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Considering the candidate 53099_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 53099_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
**** FOUND 15:17:16.75 +11:40:54.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 0.834 1169928960919576192 229.32002770564 +11.68167783238 13.6382 13.0920 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.834#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53101_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 53101_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
**** FOUND 14:53:03.54 +09:59:56.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53162_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 53162_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
**** FOUND 15:32:31.93 +18:03:54.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53212_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 53212_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
**** FOUND 15:32:31.73 +17:41:20.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53252_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 53252_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
**** FOUND 15:32:03.74 +18:02:07.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53278_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 53278_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
**** FOUND 15:32:26.39 +17:48:34.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53309_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 53309_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 53311_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 53311_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
**** FOUND 15:32:03.17 +17:58:02.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53335_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 53335_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 53356_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 53356_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 53363_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 53363_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
**** FOUND 15:31:57.28 +17:45:40.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53382_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 53382_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 53404_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 53404_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 53405_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 53405_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
**** FOUND 15:21:42.12 +14:19:22.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53466_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 53466_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
**** FOUND 14:45:44.63 +13:06:04.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 0.889 1184759929669155072 221.43571615323 +13.10117713289 12.6128 11.7146 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.889#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53507_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 53507_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 53509_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 53509_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
**** FOUND 15:31:55.87 +18:03:31.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53579_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 53579_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
**** FOUND 15:30:59.43 +12:00:18.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53620_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 53620_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
**** FOUND 15:31:43.33 +17:45:25.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53646_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 53646_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
**** FOUND 15:30:56.36 +11:54:20.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53691_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 53691_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
**** FOUND 15:24:58.80 +12:55:28.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 0.090 1170533932833422976 231.24500475657 +12.92444769040 13.6591 12.9819 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.090#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53755_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 53755_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
**** FOUND 15:19:27.75 +16:20:18.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53774_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 53774_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
**** FOUND 14:52:31.35 +17:45:07.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)GAIADR2_OUTPUT=# 3.311 1188349109284203648 223.13075549870 +17.75125535427 13.6164 13.0275 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.311#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53805_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 53805_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
**** FOUND 15:14:29.05 +11:09:30.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.97, MAG_FAINT_SEARCH_LIMIT=14.95)GAIADR2_OUTPUT=# 3.263 1168382532174865152 228.62196150549 +11.15861070584 14.2782 13.7931 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.263#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53836_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 53836_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
**** FOUND 15:32:18.52 +18:01:49.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.03, MAG_FAINT_SEARCH_LIMIT=15.01)GAIADR2_OUTPUT=# 0.302 1209535293897438720 233.07718015579 +18.03033377233 13.9679 13.4747 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.302#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53938_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 53938_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
**** FOUND 15:32:26.33 +17:31:09.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 1.218 1209294397771804288 233.11006294439 +17.51923202182 14.1436 13.5269 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.218#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53978_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 53978_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
**** FOUND 15:31:35.63 +17:25:59.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.30, MAG_FAINT_SEARCH_LIMIT=15.28)GAIADR2_OUTPUT=# 3.936 1207803253846341120 232.89950597510 +17.43349877587 14.7597 14.2686 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.936#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54019_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 54019_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
**** FOUND 15:32:21.32 +17:54:27.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 1.274 1209533163593651072 233.08914071363 +17.90772716631 14.1576 13.4965 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.274#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54083_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 54083_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
**** FOUND 15:15:07.29 +14:07:11.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)GAIADR2_OUTPUT=# 1.619 1183050429606271104 228.78022115659 +14.11932569471 14.6076 14.0469 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.619#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54097_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 54097_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 54144_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 54144_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 54153_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 54153_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
**** FOUND 15:20:01.05 +10:13:18.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.79, MAG_FAINT_SEARCH_LIMIT=15.77)GAIADR2_OUTPUT=# 2.041 1168778184562337280 230.00383997620 +10.22151165422 14.7800 14.2581 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.041#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54193_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 54193_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
**** FOUND 15:32:22.59 +17:24:33.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.62, MAG_FAINT_SEARCH_LIMIT=15.60)GAIADR2_OUTPUT=# 1.577 1209288968933138944 233.09456738036 +17.40933971745 14.7083 14.2502 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.577#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54273_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 54273_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
**** FOUND 15:14:21.77 +11:15:23.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.84, MAG_FAINT_SEARCH_LIMIT=15.82)GAIADR2_OUTPUT=# 1.448 1168397302566595328 228.59093719778 +11.25686164679 14.8739 14.3077 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.448#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54275_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 54275_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
**** FOUND 15:30:06.81 +18:03:09.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.54, MAG_FAINT_SEARCH_LIMIT=15.52)GAIADR2_OUTPUT=# 1.964 1209571302903204992 232.52894380239 +18.05273890497 14.5985 14.0767 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.964#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54303_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 54303_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
**** FOUND 15:16:20.29 +11:27:22.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.81, MAG_FAINT_SEARCH_LIMIT=15.79)GAIADR2_OUTPUT=# 0.500 1169896319168060800 229.08468042725 +11.45608281145 14.9385 14.4589 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.500#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54317_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 54317_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks
**** FOUND 15:22:29.34 +10:12:22.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.79, MAG_FAINT_SEARCH_LIMIT=15.77)GAIADR2_OUTPUT=# 1.414 1168789660715018624 230.62263385288 +10.20614257470 14.8683 14.3013 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.414#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 33946_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539
The candidate 33946_fd_Boo-10-Q2b1x1_2026-03-26_01-57-39_20.00sec_-10.00C_LIGHT_0539 did not pass the final checks