This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu
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 29.1408* 04 26 39.70 +23 11 19.5 11.8 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,2461128.6408,11.81,0.05,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 20260329.1408 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:26:39.70 +23:11:19.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20_00sec_-14_90C_LIGHT_0161_fits__*pix.png resample_wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20_00sec_-15_00C_LIGHT_0092_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20_00sec_-14_90C_LIGHT_0161_fits__*pix.png resample_wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20_00sec_-14_90C_LIGHT_0091_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20_00sec_-14_90C_LIGHT_0161_fits__*pix.png resample_wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20_00sec_-15_00C_LIGHT_0092_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20_00sec_-14_90C_LIGHT_0161_fits__*pix.png resample_wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20_00sec_-14_90C_LIGHT_0091_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 29.1408* 04 17 18.37 +23 13 52.4 13.2 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,2461128.6408,13.22,0.05,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 20260329.1408 13.22CV 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-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:17:18.37 +23:13:52.4 ;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-03-Q2b1x1_2026-01-08_22-33-15_20_00sec_-14_90C_LIGHT_0161_fits__*pix.png resample_wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20_00sec_-15_00C_LIGHT_0092_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20_00sec_-14_90C_LIGHT_0161_fits__*pix.png resample_wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20_00sec_-14_90C_LIGHT_0091_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20_00sec_-14_90C_LIGHT_0161_fits__*pix.png resample_wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20_00sec_-15_00C_LIGHT_0092_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20_00sec_-14_90C_LIGHT_0161_fits__*pix.png resample_wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20_00sec_-14_90C_LIGHT_0091_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 29.1408* 04 47 19.80 +18 57 56.7 14.1 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,2461128.6408,14.07,0.05,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 20260329.1408 14.07CV 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-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:47:19.80 +18:57:56.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20_00sec_-14_90C_LIGHT_0161_fits__*pix.png resample_wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20_00sec_-15_00C_LIGHT_0092_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20_00sec_-14_90C_LIGHT_0161_fits__*pix.png resample_wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20_00sec_-14_90C_LIGHT_0091_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20_00sec_-14_90C_LIGHT_0161_fits__*pix.png resample_wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20_00sec_-15_00C_LIGHT_0092_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20_00sec_-14_90C_LIGHT_0161_fits__*pix.png resample_wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20_00sec_-14_90C_LIGHT_0091_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 29.1408* 04 50 43.51 +21 09 19.4 14.5 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,2461128.6408,14.52,0.05,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 20260329.1408 14.52CV 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-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:50:43.51 +21:09:19.4 ;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-03-Q2b1x1_2026-01-08_22-33-15_20_00sec_-14_90C_LIGHT_0161_fits__*pix.png resample_wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20_00sec_-15_00C_LIGHT_0092_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20_00sec_-14_90C_LIGHT_0161_fits__*pix.png resample_wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20_00sec_-14_90C_LIGHT_0091_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20_00sec_-14_90C_LIGHT_0161_fits__*pix.png resample_wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20_00sec_-15_00C_LIGHT_0092_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20_00sec_-14_90C_LIGHT_0161_fits__*pix.png resample_wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20_00sec_-14_90C_LIGHT_0091_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: 2461049.68987713 09.01.2026 04:33:15.384 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
First image: 2461049.68987713 09.01.2026 04:33:15.384 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Last image: 2461128.64107863 29.03.2026 03:22:59.194 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.49
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): 9512
Objects passed selection criteria: 9462
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 7116
Average stars matched: 6946 (97.611 %)
Memory usage VmPeak: 115952 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 Sat Mar 28 22:27:54 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: 2461049.68987713 09.01.2026 04:33:15.384 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
First image: 2461049.68987713 09.01.2026 04:33:15.384 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Last image: 2461128.64107863 29.03.2026 03:22:59.194 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 60
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.17
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: 21 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): 69427
Objects passed selection criteria: 69283
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: 54754.5
Average stars matched: 53104 (96.9856 %)
Memory usage VmPeak: 172496 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 Sat Mar 28 22:29:25 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-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits
SExtractor catalog cache: saved Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.cat to cache
SExtractor catalog cache: saved Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.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-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.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: 2461128.64056970
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits exists and is non-empty
Saving wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits to local_wcs_cache/
'wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits' -> 'local_wcs_cache/wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits'
wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits exists and is non-empty
Saving wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits to local_wcs_cache/
'wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits' -> 'local_wcs_cache/wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits'
wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits exists and is non-empty
Saving wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits to local_wcs_cache/
'wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits' -> 'local_wcs_cache/wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits'
wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits exists and is non-empty
Saving wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits to local_wcs_cache/
'wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits' -> 'local_wcs_cache/wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.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 04:36:56.001 +21:59:37.88
Second-epoch image center 04:37:14.231 +22:01:00.12
Angular distance between the image centers 0.07 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 04:36:56.001 +21:59:37.88
Second-epoch image center 04:37:14.439 +22:01:14.39
Angular distance between the image centers 0.08 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 04:37:14.231 +22:01:00.12
Second-epoch second image center 04:37:14.439 +22:01:14.39
Angular distance between the image centers 0.00404 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-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits &> /tmp/tmp.rN1iH7ZPqJ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits &> /tmp/tmp.bNSgDginnv
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits &> /tmp/tmp.XvqeeW1Nld
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits &> /tmp/tmp.3vSbCljdDY
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits and wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits and wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.cat
Found non-empty wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits and wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.cat
The reference image (wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits) and catalog (wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.cat) found
'wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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 4318 out of 11927 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.977934
a=0.000000 b=1.000000 c=22.977934
From vast_summary.log: estimated ref. image limiting mag.: -7.49
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.49
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.49
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
2.0 pix Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
2.4 pix fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits
2.4 pix fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits
Limiting magnitude estimates:
15.5 mag. Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
15.5 mag. Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
14.3 mag. fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits
14.3 mag. fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 11.5 (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.rN1iH7ZPqJ (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-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits' -> 'wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
WCS_IMAGE_NAME=wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
WCS-calibrated image found: wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Checking if the catalog wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.cat corresponding to the image wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits alredy exist and is non-empty...
Catalog wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.cat corresponding to the image wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
WCS catalog name: wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=967, passed=11927
Got 11927 stars (including 10942 good ones) from the SExtractor catalog wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.cat
util/solve_plate_with_UCAC5 got 11927 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 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 962 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits -region wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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.bNSgDginnv (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-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.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_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.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-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.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-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits' -> 'wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
WCS_IMAGE_NAME=wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
WCS-calibrated image found: wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
Checking if the catalog wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits.cat corresponding to the image wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits alredy exist and is non-empty...
Catalog wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits.cat corresponding to the image wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
WCS catalog name: wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=981, passed=12023
Got 12023 stars (including 11026 good ones) from the SExtractor catalog wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits.cat
util/solve_plate_with_UCAC5 got 12023 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 961 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 961 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: 0.32"
Excluding outliers - 960 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits -region wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.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.XvqeeW1Nld (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_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.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_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits
WCS_IMAGE_NAME=wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits
WCS-calibrated image found: wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits
Checking if the catalog wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits.cat corresponding to the image wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits.cat corresponding to the image wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits
WCS catalog name: wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=399, passed=4932
Got 4932 stars (including 4530 good ones) from the SExtractor catalog wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits.cat
util/solve_plate_with_UCAC5 got 4932 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (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 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.58"
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 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.58"
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits -region wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.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.3vSbCljdDY (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_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.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_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits
WCS_IMAGE_NAME=wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits
WCS-calibrated image found: wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits
Checking if the catalog wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits.cat corresponding to the image wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits.cat corresponding to the image wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits
WCS catalog name: wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=392, passed=4930
Got 4930 stars (including 4538 good ones) from the SExtractor catalog wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits.cat
util/solve_plate_with_UCAC5 got 4930 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (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 961 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: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.56"
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 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.57"
Estimated accuracy of the plate solution: 0.58"
Excluding outliers - 959 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits -region wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.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-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits'
Saving fully-calibrated image wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits'
Saving fully-calibrated image wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits'
Saving fully-calibrated image wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits'
Preparing the HTML report for the field Tau-03-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 20655_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
The candidate 20655_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 05:03:38.47 +23:38:48.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20657_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
The candidate 20657_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 04:23:57.75 +24:18:13.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20666_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
The candidate 20666_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 04:25:25.26 +17:54:55.3 in the exclusion list exclusion_list_bsc.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-03-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-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits
SExtractor catalog cache: saved Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.cat to cache
SExtractor catalog cache: saved Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.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-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Creating symlink local_wcs_cache/wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.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-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits exists and is non-empty
wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits exists and is non-empty
wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits exists and is non-empty
wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.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 04:36:56.001 +21:59:37.88
Second-epoch image center 04:37:14.231 +22:01:00.12
Angular distance between the image centers 0.07 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 04:36:56.001 +21:59:37.88
Second-epoch image center 04:37:14.439 +22:01:14.39
Angular distance between the image centers 0.08 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 04:37:14.231 +22:01:00.12
Second-epoch second image center 04:37:14.439 +22:01:14.39
Angular distance between the image centers 0.00404 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-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits &> /tmp/tmp.TgyWyEwq0n
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits &> /tmp/tmp.uvPBSgxIj4
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits &> /tmp/tmp.sUz3FvFJKF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits &> /tmp/tmp.akDjo6NnQl
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits and wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits and wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.cat
Found non-empty wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits and wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.cat
The reference image (wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits) and catalog (wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.cat) found
'wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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 4349 out of 86341 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.826729
a=0.000000 b=1.000000 c=22.826729
From vast_summary.log: estimated ref. image limiting mag.: -7.17
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 44 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
1.9 pix Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
2.1 pix fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits
2.1 pix fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits
Limiting magnitude estimates:
15.7 mag. Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
15.6 mag. Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
14.5 mag. fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits
14.5 mag. fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits
All-image limiting magnitude estimate: 14.5 (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.TgyWyEwq0n (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-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits' -> 'wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
WCS_IMAGE_NAME=wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
WCS-calibrated image found: wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Checking if the catalog wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.cat corresponding to the image wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits alredy exist and is non-empty...
Catalog wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.cat corresponding to the image wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
WCS catalog name: wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=6242, passed=86324
Got 86324 stars (including 79904 good ones) from the SExtractor catalog wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.cat
util/solve_plate_with_UCAC5 got 86324 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 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.37"
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 959 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits -region wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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.uvPBSgxIj4 (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-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.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_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.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-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.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-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits' -> 'wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
WCS_IMAGE_NAME=wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
WCS-calibrated image found: wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
Checking if the catalog wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits.cat corresponding to the image wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits alredy exist and is non-empty...
Catalog wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits.cat corresponding to the image wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
WCS catalog name: wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=6215, passed=85672
Got 85672 stars (including 79305 good ones) from the SExtractor catalog wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits.cat
util/solve_plate_with_UCAC5 got 85672 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 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.37"
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 958 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits -region wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.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.sUz3FvFJKF (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_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.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_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits
WCS_IMAGE_NAME=wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits
WCS-calibrated image found: wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits
Checking if the catalog wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits.cat corresponding to the image wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits.cat corresponding to the image wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits
WCS catalog name: wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=1768, passed=37454
Got 37454 stars (including 35637 good ones) from the SExtractor catalog wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits.cat
util/solve_plate_with_UCAC5 got 37454 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.55"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.55"
Estimated accuracy of the plate solution: 0.57"
Excluding outliers - 959 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits -region wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.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.akDjo6NnQl (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_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.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_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits
WCS_IMAGE_NAME=wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits
WCS-calibrated image found: wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits
Checking if the catalog wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits.cat corresponding to the image wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits.cat corresponding to the image wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits
WCS catalog name: wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits.cat
SExtractor catalog parsing summary: zero_flux=5, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=1786, passed=37231
Got 37231 stars (including 35401 good ones) from the SExtractor catalog wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits.cat
util/solve_plate_with_UCAC5 got 37231 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.54"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.54"
Estimated accuracy of the plate solution: 0.57"
Excluding outliers - 959 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits -region wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.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-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/wcs_Tau-03-Q2b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Saving fully-calibrated image wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.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_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/wcs_Tau-03-Q2b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
Saving fully-calibrated image wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.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_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-15_20.00sec_-14.90C_LIGHT_0091.fits
Saving fully-calibrated image wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.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_2026-03-28_CI_Tau-03-Q2b1x1_222537_TTUQ2b1x1_7129_fJAomtFu/wcs_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092.fits
Preparing the HTML report for the field Tau-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out102680.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out102681.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out102682.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out102683.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out102695.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out102696.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out102767.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out102822.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out102871.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out102717.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out102769.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out102875.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out102888.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
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: 3s
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Considering the candidate 102680_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
The candidate 102680_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 04:21:03.49 +22:25:16.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.06, MAG_FAINT_SEARCH_LIMIT=15.04)GAIADR2_OUTPUT=# 1.589 145652962463499264 065.26406754096 +22.42111450358 14.0083 13.4612 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.589#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 102681_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
The candidate 102681_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 04:50:48.17 +18:03:03.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 0.810 3406732123197707264 072.70093469137 +18.05090619528 13.8526 13.2376 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.810#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 102682_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
The candidate 102682_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 05:02:10.55 +18:27:06.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)
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Considering the candidate 102683_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
The candidate 102683_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 04:48:50.60 +21:05:57.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 1.972 3411888282975502336 072.21024628827 +21.09941422564 13.6464 12.8930 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.972#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 102695_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
The candidate 102695_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 05:04:18.81 +23:36:39.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 0.089 3418668077832417024 076.07840178966 +23.61102601470 13.1798 12.6121 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.089#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 102696_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
The candidate 102696_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 05:04:39.87 +23:47:35.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 0.900 3418695045930603264 076.16616659680 +23.79291968552 13.0531 12.4782 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.900#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 102699_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
The candidate 102699_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 04:26:06.00 +22:54:23.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 102701_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
The candidate 102701_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 04:23:57.76 +24:18:13.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 102713_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
The candidate 102713_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 04:28:23.67 +19:10:46.5 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 102717_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
Preparing report for the candidate 102717_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
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Considering the candidate 102732_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
The candidate 102732_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 04:21:45.31 +19:28:45.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 102739_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
The candidate 102739_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 04:42:09.74 +22:55:09.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 102749_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
The candidate 102749_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 04:26:29.18 +22:48:45.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 102751_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
The candidate 102751_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 04:12:41.69 +23:31:31.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 102756_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
The candidate 102756_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 04:26:10.80 +22:49:27.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 102760_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
The candidate 102760_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 04:57:57.12 +23:57:20.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 102763_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
The candidate 102763_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 04:57:47.81 +23:58:36.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 102764_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
The candidate 102764_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 04:34:38.46 +22:42:11.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 102767_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
The candidate 102767_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 04:55:44.32 +20:00:59.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 0.681 3408610565797447040 073.93478765565 +20.01662346011 12.7649 11.8861 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.681#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 102769_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
Preparing report for the candidate 102769_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
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Considering the candidate 102777_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
The candidate 102777_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 04:27:18.10 +23:01:28.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 102778_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
The candidate 102778_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 04:55:45.38 +19:58:59.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 102779_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
The candidate 102779_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 04:14:36.76 +20:32:28.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 102797_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
The candidate 102797_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 102798_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
The candidate 102798_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 04:19:07.14 +24:00:36.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 102802_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
The candidate 102802_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 04:21:32.67 +21:00:54.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 102804_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
The candidate 102804_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 04:28:27.05 +19:11:41.3 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 102819_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
The candidate 102819_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 04:53:15.96 +24:10:37.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 102820_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
The candidate 102820_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 04:20:33.81 +25:48:35.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 102821_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
The candidate 102821_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
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Considering the candidate 102822_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
The candidate 102822_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 04:55:16.59 +21:52:02.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 0.158 3412352654840063232 073.81916547630 +21.86743950268 13.4351 12.7712 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.158#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 102823_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
The candidate 102823_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 04:41:25.50 +18:42:18.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 102825_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
The candidate 102825_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 04:36:07.88 +21:31:43.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 102827_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
The candidate 102827_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
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Considering the candidate 102831_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
The candidate 102831_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 04:25:20.53 +22:10:33.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 102832_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
The candidate 102832_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 04:19:40.47 +23:44:18.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 102840_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
The candidate 102840_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 04:19:09.33 +24:01:34.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 102847_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
The candidate 102847_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 04:19:30.00 +21:45:13.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 102862_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
The candidate 102862_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 102871_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
The candidate 102871_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 04:36:57.93 +21:03:43.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 0.969 144689858996331392 069.24166289300 +21.06212973289 14.0665 13.3981 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.969#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 102875_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
Preparing report for the candidate 102875_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
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Considering the candidate 102882_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
The candidate 102882_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks
**** FOUND 04:30:40.64 +21:55:15.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 102888_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
Preparing report for the candidate 102888_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
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Considering the candidate 102889_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092
The candidate 102889_fd_Tau-03-Q2b1x1_2026-03-28_22-22-59_20.00sec_-15.00C_LIGHT_0092 did not pass the final checks