This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS
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 02 27.1291* 03 10 53.52 +15 31 38.0 12.6 U Ari 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,2461098.6291,12.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260227.1291 12.56CV 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/Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:10:53.52 +15:31:38.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20_00sec_-14_90C_LIGHT_0228_fits__*pix.png resample_wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20_00sec_-14_90C_LIGHT_0075_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20_00sec_-14_90C_LIGHT_0228_fits__*pix.png resample_wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20_00sec_-15_00C_LIGHT_0074_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20_00sec_-14_90C_LIGHT_0228_fits__*pix.png resample_wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20_00sec_-14_90C_LIGHT_0075_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20_00sec_-14_90C_LIGHT_0228_fits__*pix.png resample_wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20_00sec_-15_00C_LIGHT_0074_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 02 27.1291* 02 48 42.09 +12 12 53.9 13.8 U Ari 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,2461098.6291,13.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260227.1291 13.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:48:42.09 +12:12:53.9 ;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_Ari-04-Q1b1x1_2025-12-22_23-16-56_20_00sec_-14_90C_LIGHT_0228_fits__*pix.png resample_wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20_00sec_-14_90C_LIGHT_0075_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20_00sec_-14_90C_LIGHT_0228_fits__*pix.png resample_wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20_00sec_-15_00C_LIGHT_0074_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20_00sec_-14_90C_LIGHT_0228_fits__*pix.png resample_wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20_00sec_-14_90C_LIGHT_0075_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20_00sec_-14_90C_LIGHT_0228_fits__*pix.png resample_wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20_00sec_-15_00C_LIGHT_0074_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 02 27.1291* 02 51 40.70 +11 27 41.2 14.4 U Ari 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,2461098.6291,14.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260227.1291 14.40CV 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/Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:51:40.70 +11:27:41.2 ;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_Ari-04-Q1b1x1_2025-12-22_23-16-56_20_00sec_-14_90C_LIGHT_0228_fits__*pix.png resample_wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20_00sec_-14_90C_LIGHT_0075_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20_00sec_-14_90C_LIGHT_0228_fits__*pix.png resample_wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20_00sec_-15_00C_LIGHT_0074_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20_00sec_-14_90C_LIGHT_0228_fits__*pix.png resample_wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20_00sec_-14_90C_LIGHT_0075_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20_00sec_-14_90C_LIGHT_0228_fits__*pix.png resample_wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20_00sec_-15_00C_LIGHT_0074_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 02 27.1291* 02 33 57.56 +16 56 14.2 14.4 U Ari 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,2461098.6291,14.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260227.1291 14.39CV 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/Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:33:57.56 +16:56:14.2 ;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_Ari-04-Q1b1x1_2025-12-22_23-16-56_20_00sec_-14_90C_LIGHT_0228_fits__*pix.png resample_wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20_00sec_-14_90C_LIGHT_0075_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20_00sec_-14_90C_LIGHT_0228_fits__*pix.png resample_wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20_00sec_-15_00C_LIGHT_0074_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20_00sec_-14_90C_LIGHT_0228_fits__*pix.png resample_wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20_00sec_-14_90C_LIGHT_0075_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20_00sec_-14_90C_LIGHT_0228_fits__*pix.png resample_wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20_00sec_-15_00C_LIGHT_0074_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: 2461032.72020931 23.12.2025 05:16:56.084 /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits
First image: 2461032.72020931 23.12.2025 05:16:56.084 /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits
Last image: 2461098.62935288 27.02.2026 03:06:06.089 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 0
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: 2 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): 7047
Objects passed selection criteria: 7025
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 5710.25
Average stars matched: 5595.25 (97.9861 %)
Memory usage VmPeak: 113368 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Feb 26 21:08:09 CST 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: 2461032.72020931 23.12.2025 05:16:56.084 /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits
First image: 2461032.72020931 23.12.2025 05:16:56.084 /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits
Last image: 2461098.62935288 27.02.2026 03:06:06.089 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 20
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.29
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: 9 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): 39884
Objects passed selection criteria: 39798
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 33994.5
Average stars matched: 33122.8 (97.4356 %)
Memory usage VmPeak: 142572 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Feb 26 21:08:55 CST 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/TTUQ1b1x1/TTUQ1_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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits
SExtractor catalog cache: saved Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits.cat to cache
SExtractor catalog cache: saved Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.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/Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.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: 2461098.62882670
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits exists and is non-empty
Saving wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits to local_wcs_cache/
'wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits' -> 'local_wcs_cache/wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits'
wcs_Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits exists and is non-empty
Saving wcs_Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits to local_wcs_cache/
'wcs_Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits' -> 'local_wcs_cache/wcs_Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits'
wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits exists and is non-empty
Saving wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits to local_wcs_cache/
'wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits' -> 'local_wcs_cache/wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits'
wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits exists and is non-empty
Saving wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits to local_wcs_cache/
'wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits' -> 'local_wcs_cache/wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.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 02:39:59.812 +13:59:58.90
Second-epoch image center 02:40:25.465 +13:59:18.37
Angular distance between the image centers 0.10 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 02:39:59.812 +13:59:58.90
Second-epoch image center 02:40:28.092 +13:59:48.74
Angular distance between the image centers 0.11 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 02:40:25.465 +13:59:18.37
Second-epoch second image center 02:40:28.092 +13:59:48.74
Angular distance between the image centers 0.01356 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/Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits &> /tmp/tmp.I7ntVAxZIU
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits &> /tmp/tmp.uEViacR7Gm
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits &> /tmp/tmp.jD3H8PpgoQ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits &> /tmp/tmp.kPnXJ2SmQL
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits
Calibrating the magnitude scale
Found non-empty wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.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_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits and wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.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_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits and wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits.cat
Found non-empty wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits and wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits.cat
The reference image (wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits) and catalog (wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits.cat) found
'wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.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 3737 out of 7440 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.954232
a=0.000000 b=1.000000 c=22.954232
From vast_summary.log: estimated ref. image limiting mag.: -7.54
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.41
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.41
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits
2.0 pix Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits
2.1 pix fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits
2.0 pix fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits
Limiting magnitude estimates:
15.4 mag. Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits
15.4 mag. Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits
14.5 mag. fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits
14.5 mag. fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 11.6 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.I7ntVAxZIU (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits' -> 'wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits
WCS_IMAGE_NAME=wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits
WCS-calibrated image found: wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits
Checking if the catalog wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits.cat corresponding to the image wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits alredy exist and is non-empty...
Catalog wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits.cat corresponding to the image wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits
WCS catalog name: wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=532, passed=7440
Got 7440 stars (including 6901 good ones) from the SExtractor catalog wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits.cat
util/solve_plate_with_UCAC5 got 7440 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 977 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: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.28"
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits -region wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.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.uEViacR7Gm (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits' -> 'wcs_Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits
WCS_IMAGE_NAME=wcs_Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits
WCS-calibrated image found: wcs_Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits
Checking if the catalog wcs_Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits.cat corresponding to the image wcs_Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits alredy exist and is non-empty...
Catalog wcs_Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits.cat corresponding to the image wcs_Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits
WCS catalog name: wcs_Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=506, passed=7504
Got 7504 stars (including 6995 good ones) from the SExtractor catalog wcs_Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits.cat
util/solve_plate_with_UCAC5 got 7504 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
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 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.29"
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 978 stars left (next iteration limit 1075)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits -region wcs_Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.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.jD3H8PpgoQ (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_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.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_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits
WCS_IMAGE_NAME=wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits
WCS-calibrated image found: wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits
Checking if the catalog wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits.cat corresponding to the image wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits alredy exist and is non-empty...
Catalog wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits.cat corresponding to the image wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits
WCS catalog name: wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=324, passed=4019
Got 4019 stars (including 3692 good ones) from the SExtractor catalog wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits.cat
util/solve_plate_with_UCAC5 got 4019 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
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: 0.31"
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 972 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_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits -region wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.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.kPnXJ2SmQL (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_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.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_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits
WCS_IMAGE_NAME=wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits
WCS-calibrated image found: wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits
Checking if the catalog wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits.cat corresponding to the image wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits alredy exist and is non-empty...
Catalog wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits.cat corresponding to the image wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits
WCS catalog name: wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=335, passed=4000
Got 4000 stars (including 3664 good ones) from the SExtractor catalog wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits.cat
util/solve_plate_with_UCAC5 got 4000 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 977 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: 0.32"
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 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.32"
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 975 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits -region wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.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_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits'
Saving fully-calibrated image wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits'
Preparing the HTML report for the field Ari-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Ari-04-Q1b1x1 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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits
SExtractor catalog cache: saved Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits.cat to cache
SExtractor catalog cache: saved Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits
Creating symlink local_wcs_cache/wcs_Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits
Creating symlink local_wcs_cache/wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits
Creating symlink local_wcs_cache/wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.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_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits exists and is non-empty
wcs_Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits exists and is non-empty
wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits exists and is non-empty
wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.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 02:39:59.812 +13:59:58.90
Second-epoch image center 02:40:25.465 +13:59:18.37
Angular distance between the image centers 0.10 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 02:39:59.812 +13:59:58.90
Second-epoch image center 02:40:28.092 +13:59:48.74
Angular distance between the image centers 0.11 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 02:40:25.465 +13:59:18.37
Second-epoch second image center 02:40:28.092 +13:59:48.74
Angular distance between the image centers 0.01356 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/Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits &> /tmp/tmp.Xox9SMhGSb
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits &> /tmp/tmp.V6E64tq8oz
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits &> /tmp/tmp.QonMzJc3so
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits &> /tmp/tmp.Gz4nDHSfUR
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits
Calibrating the magnitude scale
Found non-empty wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.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_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits and wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.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_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits and wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits.cat
Found non-empty wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits and wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits.cat
The reference image (wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits) and catalog (wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits.cat) found
'wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.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 3764 out of 43049 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.849098
a=0.000000 b=1.000000 c=22.849098
From vast_summary.log: estimated ref. image limiting mag.: -7.29
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.56
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.56
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 17 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits
1.9 pix Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits
2.0 pix fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits
1.9 pix fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits
Limiting magnitude estimates:
15.6 mag. Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits
15.6 mag. Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits
14.7 mag. fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits
14.7 mag. fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 14.1 (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.Xox9SMhGSb (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits' -> 'wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits
WCS_IMAGE_NAME=wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits
WCS-calibrated image found: wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits
Checking if the catalog wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits.cat corresponding to the image wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits alredy exist and is non-empty...
Catalog wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits.cat corresponding to the image wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits
WCS catalog name: wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=1854, passed=43033
Got 43033 stars (including 41101 good ones) from the SExtractor catalog wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits.cat
util/solve_plate_with_UCAC5 got 43033 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 977 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: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.29"
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits -region wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ari-04-Q1b1x1_2025-12-22_23-16-56_20.00sec_-14.90C_LIGHT_0228.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.V6E64tq8oz (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits' -> 'wcs_Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits
WCS_IMAGE_NAME=wcs_Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits
WCS-calibrated image found: wcs_Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits
Checking if the catalog wcs_Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits.cat corresponding to the image wcs_Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits alredy exist and is non-empty...
Catalog wcs_Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits.cat corresponding to the image wcs_Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits
WCS catalog name: wcs_Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=1823, passed=42830
Got 42830 stars (including 40938 good ones) from the SExtractor catalog wcs_Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits.cat
util/solve_plate_with_UCAC5 got 42830 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 977 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: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.30"
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits -region wcs_Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ari-04-Q1b1x1_2025-12-22_23-18-09_20.00sec_-14.90C_LIGHT_0229.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.QonMzJc3so (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_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.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_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits
WCS_IMAGE_NAME=wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits
WCS-calibrated image found: wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits
Checking if the catalog wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits.cat corresponding to the image wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits alredy exist and is non-empty...
Catalog wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits.cat corresponding to the image wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits
WCS catalog name: wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=768, passed=25421
Got 25421 stars (including 24604 good ones) from the SExtractor catalog wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits.cat
util/solve_plate_with_UCAC5 got 25421 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.31"
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_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits -region wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.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.Gz4nDHSfUR (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_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.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_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits
WCS_IMAGE_NAME=wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits
WCS-calibrated image found: wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits
Checking if the catalog wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits.cat corresponding to the image wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits alredy exist and is non-empty...
Catalog wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits.cat corresponding to the image wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits
WCS catalog name: wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=781, passed=25478
Got 25478 stars (including 24659 good ones) from the SExtractor catalog wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits.cat
util/solve_plate_with_UCAC5 got 25478 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.32"
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits -region wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.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_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.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_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-05-20_20.00sec_-15.00C_LIGHT_0074.fits
Saving fully-calibrated image wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.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_2026-02-26_CI_Ari-04-Q1b1x1_210650_TTUQ1b1x1_25377_3ecdxafS/wcs_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075.fits
Preparing the HTML report for the field Ari-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out52952.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52953.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52955.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52956.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53031.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53047.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53073.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53078.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53079.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53114.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53214.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out52991.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53091.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53229.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53246.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
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 52952_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075
The candidate 52952_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075 did not pass the final checks
**** FOUND 02:36:41.35 +09:52:59.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.42, MAG_FAINT_SEARCH_LIMIT=15.40)GAIADR2_OUTPUT=# 0.468 24792479673482624 039.17224897248 +09.88293249863 14.3593 13.7909 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.468#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52953_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075
The candidate 52953_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075 did not pass the final checks
**** FOUND 02:15:27.52 +17:16:47.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 0.346 80515969487419008 033.86456626789 +17.27975485789 13.8258 13.3460 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.346#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52955_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075
The candidate 52955_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075 did not pass the final checks
**** FOUND 02:24:46.44 +11:35:11.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 0.986 24732487570305280 036.19377236896 +11.58667323412 13.7634 13.1791 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.986#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52956_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075
The candidate 52956_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075 did not pass the final checks
**** FOUND 02:40:33.89 +13:32:27.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 1.020 26719373801283840 040.14100594438 +13.54071269640 13.2492 12.7511 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.020#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52991_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075
Preparing report for the candidate 52991_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075
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Considering the candidate 53031_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075
The candidate 53031_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075 did not pass the final checks
**** FOUND 02:55:43.72 +14:41:32.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 1.378 32332724258381056 043.93193135282 +14.69205339315 13.2576 12.7156 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.378#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53047_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075
The candidate 53047_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075 did not pass the final checks
**** FOUND 02:18:03.66 +13:26:29.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 1.931 73996930686516608 034.51492078137 +13.44184716570 13.3815 12.8902 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.931#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53050_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075
The candidate 53050_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075 did not pass the final checks
**** FOUND 03:09:58.52 +13:40:38.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53073_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075
The candidate 53073_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075 did not pass the final checks
**** FOUND 02:55:05.98 +14:47:14.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 1.732 32522802331160448 043.77454190379 +14.78778856376 13.6610 12.9592 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.732#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53078_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075
The candidate 53078_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075 did not pass the final checks
**** FOUND 02:37:21.75 +09:34:13.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 4.598 23268453478173440 039.33934280598 +09.57045911222 13.9375 13.4046 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.598#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53079_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075
The candidate 53079_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075 did not pass the final checks
**** FOUND 02:53:56.88 +16:00:06.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 2.540 34923070574241408 043.48642712349 +16.00147543853 13.8129 13.2446 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.540#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53084_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075
The candidate 53084_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075 did not pass the final checks
**** FOUND 02:25:44.17 +10:31:28.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53091_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075
Preparing report for the candidate 53091_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075
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Considering the candidate 53114_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075
The candidate 53114_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075 did not pass the final checks
**** FOUND 02:53:51.20 +15:25:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 1.222 32637319043423104 043.46303497325 +15.43148603433 14.0092 13.2666 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.222#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53214_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075
The candidate 53214_fd_Ari-04-Q1b1x1_2026-02-26_21-06-06_20.00sec_-14.90C_LIGHT_0075 did not pass the final checks