This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy
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 26.1242* 04 21 35.23 +31 26 29.0 13.6 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461125.6242,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260326.1242 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:21:35.23 +31:26:29.0 ;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_Tau-01-Q2b1x1_2026-01-08_22-27-01_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20_00sec_-10_00C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20_00sec_-10_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20_00sec_-10_00C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20_00sec_-10_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 26.1242* 04 22 23.89 +26 31 36.1 12.5 U Tau 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
VARIABLE_NAME,2461125.6242,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260326.1242 12.47CV 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/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:22:23.89 +26:31:36.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20_00sec_-10_00C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20_00sec_-10_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20_00sec_-10_00C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20_00sec_-14_90C_LIGHT_0155_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20_00sec_-10_00C_LIGHT_0308_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: 2461049.68555112 09.01.2026 04:27:01.617 /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
First image: 2461049.68555112 09.01.2026 04:27:01.617 /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
Last image: 2461125.62447159 26.03.2026 02:59:04.345 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.50
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 10944
Objects passed selection criteria: 10906
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 8609.75
Average stars matched: 8402.25 (97.5899 %)
Memory usage VmPeak: 117324 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Mar 25 22:05:19 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: 2461049.68555112 09.01.2026 04:27:01.617 /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
First image: 2461049.68555112 09.01.2026 04:27:01.617 /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
Last image: 2461125.62447159 26.03.2026 02:59:04.345 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 70
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.14
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: 42 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): 81593
Objects passed selection criteria: 81412
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 65657.8
Average stars matched: 63606.5 (96.8758 %)
Memory usage VmPeak: 1866512 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Mar 25 22:07:05 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/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits
SExtractor catalog cache: saved Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits.cat to cache
SExtractor catalog cache: saved Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.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/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.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: 2461125.62385729
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits exists and is non-empty
Saving wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits to local_wcs_cache/
'wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits' -> 'local_wcs_cache/wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits'
wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits exists and is non-empty
Saving wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits to local_wcs_cache/
'wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits' -> 'local_wcs_cache/wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits'
wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits exists and is non-empty
Saving wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits to local_wcs_cache/
'wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits' -> 'local_wcs_cache/wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits'
wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits exists and is non-empty
Saving wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits to local_wcs_cache/
'wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits' -> 'local_wcs_cache/wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 03:59:59.648 +29:59:56.09
Second-epoch image center 04:00:22.460 +30:01:07.22
Angular distance between the image centers 0.08 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 03:59:59.648 +29:59:56.09
Second-epoch image center 04:00:24.936 +30:00:40.21
Angular distance between the image centers 0.09 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 04:00:22.460 +30:01:07.22
Second-epoch second image center 04:00:24.936 +30:00:40.21
Angular distance between the image centers 0.01167 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/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits &> /tmp/tmp.i5D9ugjv8t
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits &> /tmp/tmp.vjiCEu9l2O
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits &> /tmp/tmp.Td8fxD5lFw
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits &> /tmp/tmp.ii6gTdUPvE
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.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_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits and wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.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_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits and wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits.cat
Found non-empty wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits and wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits.cat
The reference image (wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits) and catalog (wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits.cat) found
'wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.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 6059 out of 13390 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.958785
a=0.000000 b=1.000000 c=22.958785
From vast_summary.log: estimated ref. image limiting mag.: -7.50
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.46
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.46
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
2.0 pix Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
2.4 pix fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits
2.4 pix fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits
Limiting magnitude estimates:
15.5 mag. Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
15.5 mag. Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
14.4 mag. fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits
14.4 mag. fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 11.6 (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.i5D9ugjv8t (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits' -> 'wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
WCS_IMAGE_NAME=wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
WCS-calibrated image found: wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
Checking if the catalog wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits.cat corresponding to the image wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits alredy exist and is non-empty...
Catalog wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits.cat corresponding to the image wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
WCS catalog name: wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1130, passed=13390
Got 13390 stars (including 12252 good ones) from the SExtractor catalog wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits.cat
util/solve_plate_with_UCAC5 got 13390 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits -region wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.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.vjiCEu9l2O (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits' -> 'wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
WCS_IMAGE_NAME=wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
WCS-calibrated image found: wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
Checking if the catalog wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits.cat corresponding to the image wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits alredy exist and is non-empty...
Catalog wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits.cat corresponding to the image wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
WCS catalog name: wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1130, passed=13513
Got 13513 stars (including 12361 good ones) from the SExtractor catalog wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits.cat
util/solve_plate_with_UCAC5 got 13513 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits -region wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.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.Td8fxD5lFw (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits
WCS_IMAGE_NAME=wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits
WCS-calibrated image found: wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits
Checking if the catalog wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits.cat corresponding to the image wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits.cat corresponding to the image wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits
WCS catalog name: wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=448, passed=6551
Got 6551 stars (including 6096 good ones) from the SExtractor catalog wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits.cat
util/solve_plate_with_UCAC5 got 6551 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 969 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: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
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 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.49"
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 970 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits -region wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.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.ii6gTdUPvE (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits
WCS_IMAGE_NAME=wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits
WCS-calibrated image found: wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits
Checking if the catalog wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits.cat corresponding to the image wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits.cat corresponding to the image wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits
WCS catalog name: wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=466, passed=6454
Got 6454 stars (including 5979 good ones) from the SExtractor catalog wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits.cat
util/solve_plate_with_UCAC5 got 6454 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 973 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: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
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 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.50"
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits -region wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.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_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits'
Saving fully-calibrated image wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits'
Saving fully-calibrated image wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits'
Saving fully-calibrated image wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits'
Preparing the HTML report for the field Tau-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
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 20801_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 20801_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 03:51:16.39 +33:02:05.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20805_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 20805_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 03:44:56.08 +30:22:24.1 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Tau-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits
SExtractor catalog cache: saved Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits.cat to cache
SExtractor catalog cache: saved Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
Creating symlink local_wcs_cache/wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.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_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits exists and is non-empty
wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits exists and is non-empty
wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits exists and is non-empty
wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 03:59:59.648 +29:59:56.09
Second-epoch image center 04:00:22.460 +30:01:07.22
Angular distance between the image centers 0.08 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 03:59:59.648 +29:59:56.09
Second-epoch image center 04:00:24.936 +30:00:40.21
Angular distance between the image centers 0.09 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 04:00:22.460 +30:01:07.22
Second-epoch second image center 04:00:24.936 +30:00:40.21
Angular distance between the image centers 0.01167 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/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits &> /tmp/tmp.X38Ws6oYnm
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits &> /tmp/tmp.zVQwC98iXn
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits &> /tmp/tmp.Xjuj5NbTAc
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits &> /tmp/tmp.KSXMuUFHax
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.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_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits and wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.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_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits and wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits.cat
Found non-empty wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits and wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits.cat
The reference image (wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits) and catalog (wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits.cat) found
'wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.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 6106 out of 99190 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.803967
a=0.000000 b=1.000000 c=22.803967
From vast_summary.log: estimated ref. image limiting mag.: -7.14
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.66
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.66
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 51 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.8 pix Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
1.9 pix Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
2.3 pix fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits
2.2 pix fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits
Limiting magnitude estimates:
15.7 mag. Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
15.6 mag. Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
14.6 mag. fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits
14.6 mag. fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 14.0 (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.X38Ws6oYnm (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits' -> 'wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
WCS_IMAGE_NAME=wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
WCS-calibrated image found: wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
Checking if the catalog wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits.cat corresponding to the image wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits alredy exist and is non-empty...
Catalog wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits.cat corresponding to the image wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
WCS catalog name: wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=22, blended=7855, passed=99168
Got 99168 stars (including 91148 good ones) from the SExtractor catalog wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits.cat
util/solve_plate_with_UCAC5 got 99168 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits -region wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.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.zVQwC98iXn (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits' -> 'wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
WCS_IMAGE_NAME=wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
WCS-calibrated image found: wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
Checking if the catalog wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits.cat corresponding to the image wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits alredy exist and is non-empty...
Catalog wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits.cat corresponding to the image wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
WCS catalog name: wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=25, blended=7957, passed=98800
Got 98800 stars (including 90693 good ones) from the SExtractor catalog wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits.cat
util/solve_plate_with_UCAC5 got 98800 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.36"
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits -region wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.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.Xjuj5NbTAc (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits
WCS_IMAGE_NAME=wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits
WCS-calibrated image found: wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits
Checking if the catalog wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits.cat corresponding to the image wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits.cat corresponding to the image wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits
WCS catalog name: wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=2324, passed=45874
Got 45874 stars (including 43480 good ones) from the SExtractor catalog wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits.cat
util/solve_plate_with_UCAC5 got 45874 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 973 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: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
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 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.49"
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits -region wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.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.KSXMuUFHax (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits
WCS_IMAGE_NAME=wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits
WCS-calibrated image found: wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits
Checking if the catalog wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits.cat corresponding to the image wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits.cat corresponding to the image wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits
WCS catalog name: wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=2356, passed=47019
Got 47019 stars (including 44604 good ones) from the SExtractor catalog wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits.cat
util/solve_plate_with_UCAC5 got 47019 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 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.48"
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits -region wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.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_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/wcs_Tau-01-Q2b1x1_2026-01-08_22-27-01_20.00sec_-14.90C_LIGHT_0155.fits
Saving fully-calibrated image wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/wcs_Tau-01-Q2b1x1_2026-01-08_22-27-53_20.00sec_-15.00C_LIGHT_0156.fits
Saving fully-calibrated image wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-58-11_20.00sec_-10.00C_LIGHT_0308.fits
Saving fully-calibrated image wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Tau-01-Q2b1x1_220307_TTUQ2b1x1_21440_lroIu7cy/wcs_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309.fits
Preparing the HTML report for the field Tau-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out116817.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116819.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116822.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116823.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116929.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116933.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116940.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116947.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116951.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116969.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116970.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116992.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116995.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out117001.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out117003.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out117031.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out117037.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out117046.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out117054.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out117075.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out117076.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out117091.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out117117.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out116998.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77666.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 116816_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 116816_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 04:04:36.32 +33:59:34.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 116817_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 116817_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 03:49:18.45 +28:09:30.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)GAIADR2_OUTPUT=# 2.349 70894452473401088 057.32717067853 +28.15907047988 13.7173 12.9571 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.349#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116819_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 116819_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 03:43:24.73 +28:20:45.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 2.369 71812407242548480 055.85360745758 +28.34640244290 13.7178 13.1794 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.369#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116820_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 116820_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 03:41:25.45 +25:51:02.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 116822_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 116822_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 04:09:16.84 +26:50:45.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 0.549 162617735388376832 062.32024698007 +26.84596799181 13.0526 12.4595 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.549#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116823_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 116823_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 03:42:42.35 +26:53:57.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 0.480 71082842620287104 055.67655245531 +26.89949251366 12.4275 11.8013 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.480#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116851_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 116851_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 04:10:49.12 +33:34:36.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 116874_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 116874_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 03:37:35.84 +28:26:36.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 116905_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 116905_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 04:15:31.60 +33:49:31.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 116923_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 116923_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 04:08:24.89 +32:27:44.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 116929_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 116929_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 03:55:53.09 +32:10:15.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 0.916 168827781360409600 058.97098667519 +32.17111611695 12.9907 12.3273 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.916#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116933_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 116933_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 03:44:23.92 +32:11:00.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 0.987 216681688495526016 056.09995579895 +32.18332061870 12.8639 11.9781 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.987#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116940_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 116940_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 03:44:35.50 +27:52:30.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 0.162 71574534772984448 056.14795085244 +27.87496646969 13.1458 12.5801 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.162#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116942_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 116942_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 04:13:29.58 +33:27:03.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 116947_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 116947_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 04:07:46.16 +33:41:32.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 3.019 170682932356418048 061.94142817780 +33.69270225736 13.3722 12.7341 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.019#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116948_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 116948_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 03:44:11.47 +25:53:39.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 116950_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 116950_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 03:42:21.38 +33:59:24.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 116951_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 116951_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 04:07:46.87 +33:39:13.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 1.548 170681970283760384 061.94510247436 +33.65326667806 13.2176 12.4412 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.548#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116963_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 116963_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 04:11:06.70 +33:36:14.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 116969_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 116969_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 04:11:45.33 +31:32:26.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 1.121 169089396410118400 062.93919421778 +31.54054291514 13.3664 12.7575 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.121#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116970_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 116970_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 04:00:12.50 +29:34:22.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)GAIADR2_OUTPUT=# 1.735 167300972025595264 060.05257583291 +29.57269591837 13.1038 12.1486 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.735#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116992_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 116992_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 04:03:19.43 +34:13:55.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 1.899 170940321156027008 060.83056645136 +34.23238849682 13.5582 12.8058 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.899#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116995_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 116995_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 04:24:56.27 +33:34:23.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 2.787 172745410008018432 066.23538396993 +33.57329017618 13.6643 13.0664 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.787#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116998_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
Preparing report for the candidate 116998_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
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Considering the candidate 117001_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 117001_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 03:50:54.47 +29:40:02.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 1.894 167879177703472128 057.72635681478 +29.66736487740 13.6345 13.0557 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.894#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 117003_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 117003_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 04:21:11.51 +30:56:20.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.50, MAG_FAINT_SEARCH_LIMIT=14.48)GAIADR2_OUTPUT=# 2.112 166217536457730560 065.29856803562 +30.93876196388 13.3888 12.6975 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.112#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 117013_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 117013_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 04:13:17.97 +33:49:47.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117029_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 117029_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 03:46:03.15 +28:51:33.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117031_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 117031_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 04:21:46.41 +30:12:38.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 4.792 165335560630435328 065.44425821891 +30.21178502232 13.6181 12.8988 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.792#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 117036_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 117036_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 03:51:05.91 +32:33:58.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117037_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 117037_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 04:11:38.91 +29:48:36.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 2.017 165826075958752128 062.91184961337 +29.80971541631 13.2169 12.2944 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.017#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 117038_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 117038_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 04:12:18.82 +33:14:21.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117046_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 117046_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 04:09:47.08 +32:48:51.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 3.520 169812290946322432 062.44545489115 +32.81516229437 13.8273 13.1642 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.520#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 117054_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 117054_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 03:45:35.78 +28:11:29.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 0.928 71610234541083520 056.39937473886 +28.19146593472 13.8888 13.3660 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.928#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 117056_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 117056_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 04:13:21.34 +33:28:52.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117065_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 117065_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 03:45:19.77 +26:53:24.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117070_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 117070_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 04:02:30.86 +31:30:22.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117075_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 117075_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 03:50:54.52 +29:40:22.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 1.748 167879555660591872 057.72766029432 +29.67303311322 13.9380 13.2411 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.748#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 117076_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 117076_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 03:37:14.09 +29:53:39.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 3.376 120243076946432384 054.30818982567 +29.89356580904 13.9548 13.2204 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.376#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 117080_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 117080_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 03:48:32.51 +32:16:45.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117083_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 117083_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 03:59:36.59 +31:21:51.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117088_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 117088_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 04:01:50.87 +32:12:58.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117091_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 117091_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 04:11:06.07 +33:36:48.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 1.179 169965638458841472 062.77520913328 +33.61323529468 13.8515 13.2224 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.179#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 117100_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 117100_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 03:58:59.90 +32:00:41.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117117_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 117117_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 03:59:44.24 +30:46:10.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 1.267 167713426325889920 059.93465094664 +30.76933330457 14.0141 13.3743 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.267#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 117119_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 117119_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 03:46:49.08 +30:49:19.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 72300_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 72300_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 03:47:34.41 +26:16:53.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 81784_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 81784_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 04:07:01.07 +28:53:02.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 110127_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 110127_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks
**** FOUND 03:51:16.35 +33:02:05.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52535_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309
The candidate 52535_fd_Tau-01-Q2b1x1_2026-03-25_21-59-04_20.00sec_-10.00C_LIGHT_0309 did not pass the final checks