This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB
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 21.1411* 04 15 13.21 +26 14 52.5 12.4 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,2461120.6411,12.40,0.05,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 20260321.1411 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:15:13.21 +26:14:52.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20_00sec_-15_00C_LIGHT_0314_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20_00sec_-15_00C_LIGHT_0098_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20_00sec_-15_00C_LIGHT_0314_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20_00sec_-15_00C_LIGHT_0097_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20_00sec_-15_00C_LIGHT_0314_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20_00sec_-15_00C_LIGHT_0098_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20_00sec_-15_00C_LIGHT_0314_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20_00sec_-15_00C_LIGHT_0097_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 21.1411* 04 13 14.87 +31 41 59.7 13.5 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461120.6411,13.50,0.05,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 20260321.1411 13.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:13:14.87 +31:41:59.7 ;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-01-Q2b1x1_2025-12-23_00-30-55_20_00sec_-15_00C_LIGHT_0314_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20_00sec_-15_00C_LIGHT_0098_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20_00sec_-15_00C_LIGHT_0314_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20_00sec_-15_00C_LIGHT_0097_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20_00sec_-15_00C_LIGHT_0314_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20_00sec_-15_00C_LIGHT_0098_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20_00sec_-15_00C_LIGHT_0314_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20_00sec_-15_00C_LIGHT_0097_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 21.1411* 03 42 05.62 +27 17 27.2 14.2 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,2461120.6411,14.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260321.1411 14.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:42:05.62 +27:17:27.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20_00sec_-15_00C_LIGHT_0314_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20_00sec_-15_00C_LIGHT_0098_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20_00sec_-15_00C_LIGHT_0314_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20_00sec_-15_00C_LIGHT_0097_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20_00sec_-15_00C_LIGHT_0314_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20_00sec_-15_00C_LIGHT_0098_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20_00sec_-15_00C_LIGHT_0314_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20_00sec_-15_00C_LIGHT_0097_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 21.1411* 04 05 58.65 +27 19 38.4 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,2461120.6411,14.48,0.05,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 20260321.1411 14.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:05:58.65 +27:19:38.4 ;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-01-Q2b1x1_2025-12-23_00-30-55_20_00sec_-15_00C_LIGHT_0314_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20_00sec_-15_00C_LIGHT_0098_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20_00sec_-15_00C_LIGHT_0314_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20_00sec_-15_00C_LIGHT_0097_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20_00sec_-15_00C_LIGHT_0314_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20_00sec_-15_00C_LIGHT_0098_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20_00sec_-15_00C_LIGHT_0314_fits__*pix.png resample_wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20_00sec_-15_00C_LIGHT_0097_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.77159111 23.12.2025 06:30:55.472 /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits
First image: 2461032.77159111 23.12.2025 06:30:55.472 /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits
Last image: 2461120.64143367 21.03.2026 03:23:29.869 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 7
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.54
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: 5 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): 10745
Objects passed selection criteria: 10728
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 9868.25
Average stars matched: 9685.25 (98.1456 %)
Memory usage VmPeak: 117040 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Fri Mar 20 15:05:04 CDT 2026
VaST build number 1.0rc88-352-gfa78ed9d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-20)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 20 22:28:58 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: 2461032.77159111 23.12.2025 06:30:55.472 /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits
First image: 2461032.77159111 23.12.2025 06:30:55.472 /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits
Last image: 2461120.64143367 21.03.2026 03:23:29.869 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 125
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.20
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: 33 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): 81613
Objects passed selection criteria: 81458
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 75323.8
Average stars matched: 72973.5 (96.8798 %)
Memory usage VmPeak: 1912608 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Fri Mar 20 15:05:04 CDT 2026
VaST build number 1.0rc88-352-gfa78ed9d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-20)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 20 22:30:26 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits
SExtractor catalog cache: saved Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits.cat to cache
SExtractor catalog cache: saved Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.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: 2461120.64085838
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-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits exists and is non-empty
Saving wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits to local_wcs_cache/
'wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits' -> 'local_wcs_cache/wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits'
wcs_Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits exists and is non-empty
Saving wcs_Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits to local_wcs_cache/
'wcs_Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits' -> 'local_wcs_cache/wcs_Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits'
wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits exists and is non-empty
Saving wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits to local_wcs_cache/
'wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits' -> 'local_wcs_cache/wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits'
wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits exists and is non-empty
Saving wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits to local_wcs_cache/
'wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits' -> 'local_wcs_cache/wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 03:59:59.200 +29:59:56.06
Second-epoch image center 04:00:04.832 +29:59:21.91
Angular distance between the image centers 0.02 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 03:59:59.200 +29:59:56.06
Second-epoch image center 04:00:07.346 +29:59:19.03
Angular distance between the image centers 0.03 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 04:00:04.832 +29:59:21.91
Second-epoch second image center 04:00:07.346 +29:59:19.03
Angular distance between the image centers 0.00911 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits &> /tmp/tmp.8WRf0rvh2r
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits &> /tmp/tmp.WCe8ZETVWl
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits &> /tmp/tmp.frAeIvRG9r
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits &> /tmp/tmp.8tinkV1bUP
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits and wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits and wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits.cat
Found non-empty wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits and wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits.cat
The reference image (wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits) and catalog (wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits.cat) found
'wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.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 6058 out of 13222 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.971275
a=0.000000 b=1.000000 c=22.971275
From vast_summary.log: estimated ref. image limiting mag.: -7.54
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.43
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.43
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 6 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits
2.0 pix Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits
2.4 pix fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits
2.4 pix fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits
Limiting magnitude estimates:
15.4 mag. Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits
15.4 mag. Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits
15.0 mag. fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits
15.0 mag. fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 12.1 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.8WRf0rvh2r (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.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_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits' -> 'wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits
WCS_IMAGE_NAME=wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits
WCS-calibrated image found: wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits
Checking if the catalog wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits.cat corresponding to the image wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits alredy exist and is non-empty...
Catalog wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits.cat corresponding to the image wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits
WCS catalog name: wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1090, passed=13222
Got 13222 stars (including 12120 good ones) from the SExtractor catalog wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits.cat
util/solve_plate_with_UCAC5 got 13222 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits -region wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.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.WCe8ZETVWl (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.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_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits' -> 'wcs_Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits
WCS_IMAGE_NAME=wcs_Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits
WCS-calibrated image found: wcs_Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits
Checking if the catalog wcs_Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits.cat corresponding to the image wcs_Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits alredy exist and is non-empty...
Catalog wcs_Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits.cat corresponding to the image wcs_Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits
WCS catalog name: wcs_Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1060, passed=13159
Got 13159 stars (including 12083 good ones) from the SExtractor catalog wcs_Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits.cat
util/solve_plate_with_UCAC5 got 13159 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 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits -region wcs_Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.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.frAeIvRG9r (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_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.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_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits
WCS_IMAGE_NAME=wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits
WCS-calibrated image found: wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits
Checking if the catalog wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits.cat corresponding to the image wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits.cat corresponding to the image wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits
WCS catalog name: wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=698, passed=9939
Got 9939 stars (including 9234 good ones) from the SExtractor catalog wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits.cat
util/solve_plate_with_UCAC5 got 9939 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 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.55"
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 972 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: 0.56"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits -region wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.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.8tinkV1bUP (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_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.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_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits
WCS_IMAGE_NAME=wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits
WCS-calibrated image found: wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits
Checking if the catalog wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits.cat corresponding to the image wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits.cat corresponding to the image wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits
WCS catalog name: wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=669, passed=9802
Got 9802 stars (including 9125 good ones) from the SExtractor catalog wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits.cat
util/solve_plate_with_UCAC5 got 9802 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 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.55"
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 972 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: 0.56"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits -region wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits'
Saving fully-calibrated image wcs_Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/wcs_Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits'
Saving fully-calibrated image wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits'
Saving fully-calibrated image wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits'
Preparing the HTML report for the field Tau-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20694_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 20694_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 03:44:56.08 +30:22:24.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20695_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 20695_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 03:51:16.36 +33:02:04.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20696_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 20696_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 03:42:25.58 +32:56:56.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20706_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 20706_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 03:40:07.60 +26:36:34.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20709_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 20709_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 03:39:03.19 +32:52:28.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20711_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 20711_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 04:11:42.26 +26:27:18.6 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Tau-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits
SExtractor catalog cache: saved Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits.cat to cache
SExtractor catalog cache: saved Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits
Creating symlink local_wcs_cache/wcs_Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits exists and is non-empty
wcs_Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits exists and is non-empty
wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits exists and is non-empty
wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 03:59:59.200 +29:59:56.06
Second-epoch image center 04:00:04.832 +29:59:21.91
Angular distance between the image centers 0.02 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 03:59:59.200 +29:59:56.06
Second-epoch image center 04:00:07.346 +29:59:19.03
Angular distance between the image centers 0.03 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 04:00:04.832 +29:59:21.91
Second-epoch second image center 04:00:07.346 +29:59:19.03
Angular distance between the image centers 0.00911 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits &> /tmp/tmp.ZQx1CBlJWT
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits &> /tmp/tmp.XIgdYBvPOk
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits &> /tmp/tmp.2YNn6mAxSh
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits &> /tmp/tmp.Uw5fDx1b12
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits and wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits and wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits.cat
Found non-empty wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits and wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits.cat
The reference image (wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits) and catalog (wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits.cat) found
'wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.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 6109 out of 96183 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.827346
a=0.000000 b=1.000000 c=22.827346
From vast_summary.log: estimated ref. image limiting mag.: -7.20
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.63
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.63
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 66 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits
1.9 pix Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits
2.1 pix fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits
2.1 pix fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits
Limiting magnitude estimates:
15.6 mag. Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits
15.6 mag. Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits
15.2 mag. fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits
15.2 mag. fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits
All-image limiting magnitude estimate: 15.2 (SNR ) 14.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.ZQx1CBlJWT (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.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_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits' -> 'wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits
WCS_IMAGE_NAME=wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits
WCS-calibrated image found: wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits
Checking if the catalog wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits.cat corresponding to the image wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits alredy exist and is non-empty...
Catalog wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits.cat corresponding to the image wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits
WCS catalog name: wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=21, blended=7465, passed=96162
Got 96162 stars (including 88540 good ones) from the SExtractor catalog wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits.cat
util/solve_plate_with_UCAC5 got 96162 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 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
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 973 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: 0.35"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits -region wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.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.XIgdYBvPOk (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.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_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits' -> 'wcs_Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits
WCS_IMAGE_NAME=wcs_Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits
WCS-calibrated image found: wcs_Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits
Checking if the catalog wcs_Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits.cat corresponding to the image wcs_Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits alredy exist and is non-empty...
Catalog wcs_Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits.cat corresponding to the image wcs_Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits
WCS catalog name: wcs_Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=22, blended=7415, passed=96287
Got 96287 stars (including 88726 good ones) from the SExtractor catalog wcs_Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits.cat
util/solve_plate_with_UCAC5 got 96287 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 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
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 974 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: 0.35"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits -region wcs_Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.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.2YNn6mAxSh (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_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.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_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits
WCS_IMAGE_NAME=wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits
WCS-calibrated image found: wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits
Checking if the catalog wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits.cat corresponding to the image wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits.cat corresponding to the image wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits
WCS catalog name: wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=4604, passed=69979
Got 69979 stars (including 65284 good ones) from the SExtractor catalog wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits.cat
util/solve_plate_with_UCAC5 got 69979 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 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.53"
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits -region wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.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.Uw5fDx1b12 (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_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.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_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits
WCS_IMAGE_NAME=wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits
WCS-calibrated image found: wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits
Checking if the catalog wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits.cat corresponding to the image wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits.cat corresponding to the image wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits
WCS catalog name: wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=26, blended=4625, passed=70408
Got 70408 stars (including 65687 good ones) from the SExtractor catalog wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits.cat
util/solve_plate_with_UCAC5 got 70408 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 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.56"
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 974 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: 0.55"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits -region wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.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_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/wcs_Tau-01-Q2b1x1_2025-12-23_00-30-55_20.00sec_-15.00C_LIGHT_0314.fits
Saving fully-calibrated image wcs_Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.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_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/wcs_Tau-01-Q2b1x1_2025-12-23_00-31-31_20.00sec_-15.00C_LIGHT_0315.fits
Saving fully-calibrated image wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.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_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-22-40_20.00sec_-15.00C_LIGHT_0097.fits
Saving fully-calibrated image wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.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_2026-03-20_CI_Tau-01-Q2b1x1_222424_TTUQ2b1x1_26891_irAsy6AB/wcs_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098.fits
Preparing the HTML report for the field Tau-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out113711.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out113718.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out113723.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out113733.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out113736.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out113737.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out113747.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out113748.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out113750.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out113751.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out113757.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out113760.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out113763.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out113768.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out113906.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out113960.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out113970.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out113981.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out113989.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out114044.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out114083.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out114085.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out114094.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out114119.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out114186.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out114229.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out113813.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out113926.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out114051.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out114166.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 9s
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 113711_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 113711_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 04:30:41.66 +28:01:18.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 3.309 152619330697802240 067.67322632547 +28.02269692821 13.7464 12.9859 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.309#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 113715_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 113715_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 04:23:24.08 +32:10:51.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113718_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 113718_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 04:31:07.98 +29:00:47.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.24, MAG_FAINT_SEARCH_LIMIT=15.22)
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Considering the candidate 113723_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 113723_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 03:50:08.34 +26:02:19.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.45, MAG_FAINT_SEARCH_LIMIT=15.43)GAIADR2_OUTPUT=# 0.900 69998109977324672 057.53502287801 +26.03874311847 14.3771 13.7474 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 113733_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 113733_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 04:03:01.70 +25:56:52.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)GAIADR2_OUTPUT=# 1.004 162502153527482240 060.75739348267 +25.94788399087 14.2335 13.7334 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.004#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 113736_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 113736_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 03:39:03.79 +30:04:60.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)
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Considering the candidate 113737_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 113737_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 03:34:56.37 +26:39:28.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 1.769 69721857680191616 053.73529752545 +26.65817549237 14.2102 13.5291 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.769#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 113741_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 113741_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 03:55:56.56 +34:11:22.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113747_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 113747_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 03:37:47.98 +27:22:00.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.05, MAG_FAINT_SEARCH_LIMIT=15.03)GAIADR2_OUTPUT=# 0.300 71276257884059008 054.44983232325 +27.36684238651 14.0094 13.4340 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.300#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 113748_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 113748_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 04:12:17.67 +27:47:32.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 0.493 163188076982650624 063.07358202237 +27.79257613577 13.4746 12.8773 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.493#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 113750_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 113750_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 03:44:07.49 +25:53:20.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 0.934 70132868871097856 056.03119218510 +25.88920345267 14.1859 13.5860 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.934#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 113751_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 113751_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 03:47:39.11 +27:41:00.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 1.419 70783367438085120 056.91334346359 +27.68355866469 13.6613 13.1955 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.419#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 113757_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 113757_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 03:48:04.11 +29:42:43.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 2.283 168055786758732672 057.01776666470 +29.71233064421 13.5802 12.8372 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.283#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 113758_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 113758_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 03:42:33.68 +27:33:37.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113760_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 113760_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 03:32:24.33 +30:19:09.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 0.314 120682297481789568 053.10127965083 +30.31941769818 12.8108 11.8100 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.314#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 113763_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 113763_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 03:45:00.54 +30:39:56.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 2.230 216207829046932352 056.25296821057 +30.66560145884 13.0121 12.1706 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.230#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 113764_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 113764_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 03:41:25.39 +25:51:02.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113768_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 113768_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 03:49:17.17 +26:54:51.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 1.608 70473992354767616 057.32192485736 +26.91448192920 12.6422 12.0643 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.608#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 113787_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 113787_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 03:40:07.61 +26:36:34.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113794_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 113794_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 03:39:03.23 +32:52:28.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113800_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 113800_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 03:37:35.80 +28:26:36.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113813_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
Preparing report for the candidate 113813_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
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Considering the candidate 113840_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 113840_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 04:15:31.41 +33:49:30.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113862_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 113862_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 04:15:32.73 +33:50:12.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113876_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 113876_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 03:40:32.25 +29:55:51.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113878_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 113878_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 04:08:24.87 +32:27:45.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113906_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 113906_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 04:13:29.62 +33:27:04.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)
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Considering the candidate 113922_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 113922_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 03:44:11.42 +25:53:40.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113926_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
Preparing report for the candidate 113926_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
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Considering the candidate 113936_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 113936_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 03:46:03.10 +28:51:33.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113943_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 113943_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 04:13:17.83 +33:49:47.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113945_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 113945_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 03:45:19.69 +26:53:23.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113960_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 113960_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 04:03:56.96 +25:50:59.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 1.983 162490746094533248 060.98793073969 +25.85003715286 13.7288 13.2274 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.983#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 113970_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 113970_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 04:13:21.09 +33:28:50.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)GAIADR2_OUTPUT=# 4.049 169928461222245760 063.33902158946 +33.48134182336 13.3840 12.5395 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.049#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 113981_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 113981_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 03:50:32.60 +33:35:16.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 2.094 217264738897607296 057.63652756709 +33.58788150908 13.9533 13.3147 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.094#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 113984_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 113984_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 03:51:05.99 +32:33:58.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113989_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 113989_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 04:12:18.70 +33:14:19.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 2.150 169895647672291072 063.07859360286 +33.23850439451 13.9852 13.7178 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.150#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 114013_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 114013_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 03:59:36.52 +31:21:51.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 114021_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 114021_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 03:37:47.33 +29:13:29.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 114024_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 114024_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 04:01:50.65 +32:12:57.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 114036_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 114036_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 03:46:03.00 +27:20:18.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 114044_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 114044_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 04:08:08.32 +30:50:05.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.97, MAG_FAINT_SEARCH_LIMIT=14.95)GAIADR2_OUTPUT=# 2.913 168946391177936512 062.03373242583 +30.83493867872 13.6455 12.6682 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.913#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 114051_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
Preparing report for the candidate 114051_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
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Considering the candidate 114056_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 114056_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 04:22:39.90 +32:28:48.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 114074_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 114074_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 03:57:07.84 +32:01:49.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 114083_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 114083_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 03:46:49.10 +30:49:19.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 1.223 216236764243553280 056.70475318076 +30.82241807132 14.1015 13.4129 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.223#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 114085_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 114085_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 03:40:42.06 +34:02:45.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.41, MAG_FAINT_SEARCH_LIMIT=15.39)GAIADR2_OUTPUT=# 0.593 218218565234033280 055.17544425786 +34.04611851172 13.9409 13.2763 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.593#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 114094_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 114094_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 04:03:03.10 +28:26:47.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 2.631 164175300987219840 060.76374089590 +28.44651748885 13.8821 13.1297 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.631#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 114098_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 114098_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 03:38:40.93 +28:22:12.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 114116_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 114116_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 04:05:37.82 +31:48:56.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 114119_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 114119_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 03:50:38.18 +26:41:42.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.19, MAG_FAINT_SEARCH_LIMIT=15.17)GAIADR2_OUTPUT=# 1.515 70475194945790464 057.65954598677 +26.69521767517 14.3393 13.8614 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.515#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 114141_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 114141_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 03:36:00.29 +30:05:51.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 114165_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 114165_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 04:07:46.35 +33:57:52.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 114166_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
Preparing report for the candidate 114166_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
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Considering the candidate 114182_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 114182_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 03:45:17.69 +30:15:44.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 114186_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 114186_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 03:44:18.38 +29:10:09.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.37, MAG_FAINT_SEARCH_LIMIT=15.35)GAIADR2_OUTPUT=# 2.154 71996128762836224 056.07718951365 +29.16969545927 14.5067 14.0136 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.154#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 114204_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 114204_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 04:09:11.44 +32:04:10.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 114229_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 114229_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 03:49:52.40 +26:47:52.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.45, MAG_FAINT_SEARCH_LIMIT=15.43)GAIADR2_OUTPUT=# 1.305 70491962497939584 057.46872472348 +26.79790195659 14.7236 14.1281 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.305#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107877_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 107877_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 03:51:16.35 +33:02:04.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108078_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 108078_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 03:34:37.86 +28:15:37.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 38924_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 38924_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
Rejecting candidate due to large distance (32.0") between the two second-epoch detections
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Considering the candidate 51022_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 51022_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 03:44:56.06 +30:22:24.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70030_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 70030_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
**** FOUND 03:47:34.36 +26:16:53.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 50281_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 50281_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
Rejecting candidate due to large distance (32.4") between the two second-epoch detections
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Considering the candidate 21965_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 21965_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks
Rejecting candidate due to large distance (31.1") between the two second-epoch detections
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Considering the candidate 112170_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098
The candidate 112170_fd_Tau-01-Q2b1x1_2026-03-20_22-23-29_20.00sec_-15.00C_LIGHT_0098 did not pass the final checks