This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo
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 12.1304* 01 18 10.47 +01 12 08.5 9.2 U Cet 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,2461083.6304,9.19,0.05,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 20260212.1304 9.19CV 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/Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:18:10.47 +01:12:08.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20_00sec_-15_00C_LIGHT_0131_fits__*pix.png resample_wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20_00sec_-15_00C_LIGHT_0070_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20_00sec_-15_00C_LIGHT_0131_fits__*pix.png resample_wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20_00sec_-14_90C_LIGHT_0069_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20_00sec_-15_00C_LIGHT_0131_fits__*pix.png resample_wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20_00sec_-15_00C_LIGHT_0070_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20_00sec_-15_00C_LIGHT_0131_fits__*pix.png resample_wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20_00sec_-14_90C_LIGHT_0069_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 12.1304* 01 15 09.62 -04 57 20.3 10.2 U Cet 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,2461083.6304,10.19,0.05,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 20260212.1304 10.19CV 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/Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:15:09.62 -04:57:20.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20_00sec_-15_00C_LIGHT_0131_fits__*pix.png resample_wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20_00sec_-15_00C_LIGHT_0070_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20_00sec_-15_00C_LIGHT_0131_fits__*pix.png resample_wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20_00sec_-14_90C_LIGHT_0069_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20_00sec_-15_00C_LIGHT_0131_fits__*pix.png resample_wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20_00sec_-15_00C_LIGHT_0070_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20_00sec_-15_00C_LIGHT_0131_fits__*pix.png resample_wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20_00sec_-14_90C_LIGHT_0069_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 12.1304* 01 31 52.84 +00 29 07.6 14.2 U Cet 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,2461083.6304,14.21,0.05,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 20260212.1304 14.21CV 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/Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:31:52.84 -00:29:07.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20_00sec_-15_00C_LIGHT_0131_fits__*pix.png resample_wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20_00sec_-15_00C_LIGHT_0070_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20_00sec_-15_00C_LIGHT_0131_fits__*pix.png resample_wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20_00sec_-14_90C_LIGHT_0069_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20_00sec_-15_00C_LIGHT_0131_fits__*pix.png resample_wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20_00sec_-15_00C_LIGHT_0070_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20_00sec_-15_00C_LIGHT_0131_fits__*pix.png resample_wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20_00sec_-14_90C_LIGHT_0069_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 12.1304* 01 22 23.63 -01 37 18.1 14.3 U Cet 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,2461083.6304,14.31,0.05,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 20260212.1304 14.31CV 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/Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 01:22:23.63 -01:37:18.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20_00sec_-15_00C_LIGHT_0131_fits__*pix.png resample_wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20_00sec_-15_00C_LIGHT_0070_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20_00sec_-15_00C_LIGHT_0131_fits__*pix.png resample_wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20_00sec_-14_90C_LIGHT_0069_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20_00sec_-15_00C_LIGHT_0131_fits__*pix.png resample_wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20_00sec_-15_00C_LIGHT_0070_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20_00sec_-15_00C_LIGHT_0131_fits__*pix.png resample_wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20_00sec_-14_90C_LIGHT_0069_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: 2461032.65469490 23.12.2025 03:42:35.639 /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits
First image: 2461032.65469490 23.12.2025 03:42:35.639 /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits
Last image: 2461083.63064917 12.02.2026 03:07:58.088 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 14
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.64
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 5880
Objects passed selection criteria: 5876
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 5342.75
Average stars matched: 5249.5 (98.2546 %)
Memory usage VmPeak: 112228 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 Wed Feb 11 21:11:09 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: 2461032.65469490 23.12.2025 03:42:35.639 /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits
First image: 2461032.65469490 23.12.2025 03:42:35.639 /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits
Last image: 2461083.63064917 12.02.2026 03:07:58.088 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 80
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.41
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: 13 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): 30985
Objects passed selection criteria: 30926
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 29190.2
Average stars matched: 28473.2 (97.5437 %)
Memory usage VmPeak: 134124 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 Wed Feb 11 21:12:10 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/Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits
SExtractor catalog cache: saved Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits.cat to cache
SExtractor catalog cache: saved Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.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/Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.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: 2461083.63012072
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits exists and is non-empty
Saving wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits to local_wcs_cache/
'wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits' -> 'local_wcs_cache/wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits'
wcs_Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits exists and is non-empty
Saving wcs_Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits to local_wcs_cache/
'wcs_Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits' -> 'local_wcs_cache/wcs_Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits'
wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits exists and is non-empty
Saving wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits to local_wcs_cache/
'wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits' -> 'local_wcs_cache/wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits'
wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits exists and is non-empty
Saving wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits to local_wcs_cache/
'wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits' -> 'local_wcs_cache/wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.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 01:42:37.582 -02:00:52.43
Second-epoch image center 01:42:38.201 -02:00:14.32
Angular distance between the image centers 0.01 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 01:42:37.582 -02:00:52.43
Second-epoch image center 01:42:40.928 -02:00:45.78
Angular distance between the image centers 0.01 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 01:42:38.201 -02:00:14.32
Second-epoch second image center 01:42:40.928 -02:00:45.78
Angular distance between the image centers 0.01433 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/Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits &> /tmp/tmp.zj40vig4nZ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits &> /tmp/tmp.uJk0ogeGYm
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits &> /tmp/tmp.EjpyRRPymA
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits &> /tmp/tmp.Mf8zRke4uF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits
Calibrating the magnitude scale
Found non-empty wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.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_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits and wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.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_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits and wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits.cat
Found non-empty wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits and wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits.cat
The reference image (wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits) and catalog (wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits.cat) found
'wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.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 3552 out of 6231 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.928968
a=0.000000 b=1.000000 c=22.928968
From vast_summary.log: estimated ref. image limiting mag.: -7.64
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.29
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.29
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 10 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits
2.0 pix Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits
2.0 pix fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits
2.0 pix fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits
Limiting magnitude estimates:
15.3 mag. Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits
15.3 mag. Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits
14.8 mag. fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits
14.8 mag. fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 11.8 (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.zj40vig4nZ (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_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits' -> 'wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits
WCS_IMAGE_NAME=wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits
WCS-calibrated image found: wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits
Checking if the catalog wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits.cat corresponding to the image wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits alredy exist and is non-empty...
Catalog wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits.cat corresponding to the image wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits
WCS catalog name: wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=449, passed=6231
Got 6231 stars (including 5767 good ones) from the SExtractor catalog wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits.cat
util/solve_plate_with_UCAC5 got 6231 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 981 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: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.27"
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 981 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.26"
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 980 stars left (next iteration limit 1078)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits -region wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.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.uJk0ogeGYm (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_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits' -> 'wcs_Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits
WCS_IMAGE_NAME=wcs_Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits
WCS-calibrated image found: wcs_Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits
Checking if the catalog wcs_Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits.cat corresponding to the image wcs_Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits alredy exist and is non-empty...
Catalog wcs_Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits.cat corresponding to the image wcs_Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits
WCS catalog name: wcs_Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=445, passed=6235
Got 6235 stars (including 5783 good ones) from the SExtractor catalog wcs_Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits.cat
util/solve_plate_with_UCAC5 got 6235 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 980 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: 0.27"
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 980 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.27"
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 979 stars left (next iteration limit 1076)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits -region wcs_Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.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.EjpyRRPymA (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_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.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_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits
WCS_IMAGE_NAME=wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits
WCS-calibrated image found: wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits
Checking if the catalog wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits.cat corresponding to the image wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits alredy exist and is non-empty...
Catalog wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits.cat corresponding to the image wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits
WCS catalog name: wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=331, passed=4522
Got 4522 stars (including 4184 good ones) from the SExtractor catalog wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits.cat
util/solve_plate_with_UCAC5 got 4522 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.1'
Seting catalog search parameters based on the expected field of view 942.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013085 (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 0.010468 (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: 0.32"
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 974 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: 0.31"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits -region wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.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.Mf8zRke4uF (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_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.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_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits
WCS_IMAGE_NAME=wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits
WCS-calibrated image found: wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits
Checking if the catalog wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits.cat corresponding to the image wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits alredy exist and is non-empty...
Catalog wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits.cat corresponding to the image wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits
WCS catalog name: wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=329, passed=4525
Got 4525 stars (including 4190 good ones) from the SExtractor catalog wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits.cat
util/solve_plate_with_UCAC5 got 4525 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.1'
Seting catalog search parameters based on the expected field of view 942.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013085 (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 0.010468 (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: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits -region wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.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_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits'
Saving fully-calibrated image wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits'
Preparing the HTML report for the field Cet-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20353.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20356.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20357.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20359.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20362.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20363.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out20347.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20351.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
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: 2s
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Considering the candidate 20346_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 20346_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:12:47.65 -06:46:60.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 20347_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
Preparing report for the candidate 20347_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20351_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
Preparing report for the candidate 20351_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20353_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 20353_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:12:13.63 -06:39:16.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.24, MAG_FAINT_SEARCH_LIMIT=12.22)GAIADR2_OUTPUT=# 0.200 2475793735540082688 018.05683468307 -06.65456308518 10.9138 10.3379 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.200#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20356_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 20356_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:12:16.90 -07:04:40.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.52, MAG_FAINT_SEARCH_LIMIT=12.50)GAIADR2_OUTPUT=# 0.935 2475624616908499200 018.07021818395 -07.07808608991 11.0681 10.2541 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.935#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20357_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 20357_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:12:07.88 -06:39:56.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.65, MAG_FAINT_SEARCH_LIMIT=12.63)GAIADR2_OUTPUT=# 0.367 2475793701181120384 018.03274518378 -06.66560792035 11.2504 10.5742 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.367#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20359_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 20359_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:12:30.12 -06:48:08.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 0.613 2475738278923143936 018.12566904666 -06.80238904817 11.4836 10.6963 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.613#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20362_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 20362_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:13:05.29 -06:51:29.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 0.570 2475739614657320704 018.27219617165 -06.85812754475 11.8232 11.3149 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.570#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20363_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 20363_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:12:29.92 -06:50:38.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 0.875 2475737557368640000 018.12485060076 -06.84375619833 11.8044 11.3115 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.875#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 00210_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 00210_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:30:38.37 +02:52:49.4 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 8s
Prepared the HTML report for the field Cet-03-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 ####
01:18:10.47 +01:12:08.5
01:15:09.62 -04:57:20.3
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/Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits
SExtractor catalog cache: saved Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits.cat to cache
SExtractor catalog cache: saved Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits
Creating symlink local_wcs_cache/wcs_Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits
Creating symlink local_wcs_cache/wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits
Creating symlink local_wcs_cache/wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.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_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits exists and is non-empty
wcs_Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits exists and is non-empty
wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits exists and is non-empty
wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.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 01:42:37.582 -02:00:52.43
Second-epoch image center 01:42:38.201 -02:00:14.32
Angular distance between the image centers 0.01 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 01:42:37.582 -02:00:52.43
Second-epoch image center 01:42:40.928 -02:00:45.78
Angular distance between the image centers 0.01 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 01:42:38.201 -02:00:14.32
Second-epoch second image center 01:42:40.928 -02:00:45.78
Angular distance between the image centers 0.01433 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/Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits &> /tmp/tmp.B9ZCdNUjLy
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits &> /tmp/tmp.62wHtPQrQE
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits &> /tmp/tmp.HRq1gfqr2x
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits &> /tmp/tmp.RumPQoW8Cq
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits
Calibrating the magnitude scale
Found non-empty wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.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_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits and wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.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_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits and wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits.cat
Found non-empty wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits and wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits.cat
The reference image (wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits) and catalog (wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits.cat) found
'wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.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 3586 out of 32735 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.837246
a=0.000000 b=1.000000 c=22.837246
From vast_summary.log: estimated ref. image limiting mag.: -7.41
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.43
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.43
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 54 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits
1.9 pix Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits
1.9 pix fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits
1.9 pix fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits
Limiting magnitude estimates:
15.4 mag. Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits
15.4 mag. Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits
15.0 mag. fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits
15.0 mag. fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 14.4 (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.B9ZCdNUjLy (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_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits' -> 'wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits
WCS_IMAGE_NAME=wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits
WCS-calibrated image found: wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits
Checking if the catalog wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits.cat corresponding to the image wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits alredy exist and is non-empty...
Catalog wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits.cat corresponding to the image wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits
WCS catalog name: wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=1285, passed=32717
Got 32717 stars (including 31362 good ones) from the SExtractor catalog wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits.cat
util/solve_plate_with_UCAC5 got 32717 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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: 0.28"
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 978 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 - 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_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits -region wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cet-03-Q1b1x1_2025-12-22_21-42-35_20.00sec_-15.00C_LIGHT_0131.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.62wHtPQrQE (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_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits' -> 'wcs_Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits
WCS_IMAGE_NAME=wcs_Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits
WCS-calibrated image found: wcs_Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits
Checking if the catalog wcs_Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits.cat corresponding to the image wcs_Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits alredy exist and is non-empty...
Catalog wcs_Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits.cat corresponding to the image wcs_Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits
WCS catalog name: wcs_Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=1310, passed=32658
Got 32658 stars (including 31302 good ones) from the SExtractor catalog wcs_Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits.cat
util/solve_plate_with_UCAC5 got 32658 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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: 0.29"
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 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: 0.27"
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_Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits -region wcs_Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cet-03-Q1b1x1_2025-12-22_21-43-19_20.00sec_-15.00C_LIGHT_0132.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.HRq1gfqr2x (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_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.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_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits
WCS_IMAGE_NAME=wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits
WCS-calibrated image found: wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits
Checking if the catalog wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits.cat corresponding to the image wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits alredy exist and is non-empty...
Catalog wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits.cat corresponding to the image wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits
WCS catalog name: wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=802, passed=26061
Got 26061 stars (including 25216 good ones) from the SExtractor catalog wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits.cat
util/solve_plate_with_UCAC5 got 26061 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.1'
Seting catalog search parameters based on the expected field of view 942.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013085 (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 0.010468 (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: 0.33"
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 975 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 - 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_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits -region wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.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.RumPQoW8Cq (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_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.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_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits
WCS_IMAGE_NAME=wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits
WCS-calibrated image found: wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits
Checking if the catalog wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits.cat corresponding to the image wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits alredy exist and is non-empty...
Catalog wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits.cat corresponding to the image wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits
WCS catalog name: wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=829, passed=25981
Got 25981 stars (including 25112 good ones) from the SExtractor catalog wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits.cat
util/solve_plate_with_UCAC5 got 25981 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.1'
Seting catalog search parameters based on the expected field of view 942.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013085 (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 0.010468 (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 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits -region wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.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_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.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_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-12_20.00sec_-14.90C_LIGHT_0069.fits
Saving fully-calibrated image wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.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_2026-02-11_CI_Cet-03-Q1b1x1_210844_TTUQ1b1x1_18391_afSVgJqo/wcs_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070.fits
Preparing the HTML report for the field Cet-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out52150.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52153.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52156.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52157.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52161.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52162.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52169.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52170.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52171.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52174.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52178.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52188.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52189.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52190.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52192.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52195.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52206.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52208.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52211.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52218.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52222.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52224.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52225.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52228.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52230.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52233.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52239.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52241.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52250.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52261.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52262.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52267.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52277.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52278.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52282.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52283.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52286.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52294.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52298.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52308.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52315.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52317.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52320.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52322.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out52313.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52328.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 10s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52143_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52143_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:12:47.64 -06:47:00.1 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52144_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52144_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:18:10.47 +01:12:08.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52148_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52148_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:15:09.63 -04:57:20.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52150_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52150_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:13:52.47 -07:02:29.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.43, MAG_FAINT_SEARCH_LIMIT=11.41)GAIADR2_OUTPUT=# 0.899 2475528340921595904 018.46852003218 -07.04124533656 10.2416 9.7558 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.899#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52153_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52153_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:12:13.61 -06:39:16.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.11, MAG_FAINT_SEARCH_LIMIT=12.09)GAIADR2_OUTPUT=# 0.458 2475793735540082688 018.05683468307 -06.65456308518 10.9138 10.3379 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.458#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52156_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52156_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:12:16.88 -07:04:40.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.38, MAG_FAINT_SEARCH_LIMIT=12.36)GAIADR2_OUTPUT=# 0.462 2475624616908499200 018.07021818395 -07.07808608991 11.0681 10.2541 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.462#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52157_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52157_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:12:07.87 -06:39:56.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.51, MAG_FAINT_SEARCH_LIMIT=12.49)GAIADR2_OUTPUT=# 0.167 2475793701181120384 018.03274518378 -06.66560792035 11.2504 10.5742 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.167#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52161_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52161_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:12:30.10 -06:48:08.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.75, MAG_FAINT_SEARCH_LIMIT=12.73)GAIADR2_OUTPUT=# 0.924 2475738278923143936 018.12566904666 -06.80238904817 11.4836 10.6963 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.924#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52162_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52162_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:13:35.80 -06:50:12.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.78, MAG_FAINT_SEARCH_LIMIT=12.76)GAIADR2_OUTPUT=# 0.866 2475728172864443904 018.39937499501 -06.83662714947 11.5985 11.0614 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.866#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52169_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52169_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:13:05.29 -06:51:29.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)GAIADR2_OUTPUT=# 0.707 2475739614657320704 018.27219617165 -06.85812754475 11.8232 11.3149 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.707#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52170_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52170_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:12:29.90 -06:50:38.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.97, MAG_FAINT_SEARCH_LIMIT=12.95)GAIADR2_OUTPUT=# 1.367 2475737557368640000 018.12485060076 -06.84375619833 11.8044 11.3115 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.367#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52171_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52171_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:13:16.55 -06:44:01.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 0.136 2475743158006003968 018.31899621820 -06.73364033622 11.8082 11.1377 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.136#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52174_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52174_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:11:51.80 -06:36:16.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 0.651 2475797888773394688 017.96597525732 -06.60447024971 11.9815 11.2912 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.651#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52178_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52178_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:12:31.36 -06:59:47.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 0.455 2475730887283775872 018.13073585236 -06.99650510157 12.0971 11.4131 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.455#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52188_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52188_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:12:16.85 -07:05:51.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 0.767 2475624513829284352 018.07038748333 -07.09763237175 12.3279 11.7855 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.767#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52189_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52189_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:13:12.45 -06:40:38.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 0.444 2475746383525775744 018.30197916385 -06.67718284692 12.4658 11.8845 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.444#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52190_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52190_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:14:24.19 -06:58:29.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 1.017 2475536174941943424 018.60050702759 -06.97483175908 12.4668 11.9197 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.017#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52192_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52192_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:11:56.92 -06:34:46.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 0.825 2475798030508153984 017.98739720611 -06.57970002741 12.4895 12.0016 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.825#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52195_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52195_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:12:41.92 -07:06:33.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.75, MAG_FAINT_SEARCH_LIMIT=13.73)GAIADR2_OUTPUT=# 1.084 2475623689195564672 018.17497011791 -07.10917479331 12.5772 12.0896 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.084#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52206_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52206_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:13:59.27 -06:49:36.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 0.992 2475729173592505088 018.49674437162 -06.82684209268 12.6046 12.0244 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.992#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52208_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52208_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:12:13.37 -07:04:19.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 0.044 2475636367939020928 018.05570344360 -07.07204434509 12.5653 11.9273 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.044#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52211_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52211_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:14:46.56 -07:02:22.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 0.995 2475531879974662912 018.69377094546 -07.03971265893 12.8311 12.3431 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.995#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52218_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52218_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:14:22.41 -07:07:16.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 1.426 2475529577872179584 018.59298816024 -07.12106841339 13.0760 12.4156 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.426#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52222_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52222_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:13:52.60 -06:49:05.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.25, MAG_FAINT_SEARCH_LIMIT=14.23)GAIADR2_OUTPUT=# 0.788 2475729001793812864 018.46922442624 -06.81809434782 12.9694 12.2794 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.788#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52224_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52224_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:51:30.50 -01:35:01.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 1.196 2505791294669425280 027.87682759194 -01.58385086712 13.5063 12.9431 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.196#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52225_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52225_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:13:05.52 -06:26:45.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 0.653 2475820845374463104 018.27282538574 -06.44608072483 13.1998 12.6631 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.653#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52228_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52228_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:12:15.91 -06:44:45.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 0.284 2475786313837371648 018.06637074155 -06.74585435756 13.2149 12.6353 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.284#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52230_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52230_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:11:57.65 -06:23:03.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 1.577 2475814145225452800 017.99064238983 -06.38428467936 13.2015 12.4468 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.577#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52233_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52233_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:13:08.44 -07:02:06.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 0.921 2475715322322295552 018.28503356791 -07.03503085422 12.7792 11.6515 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.921#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52239_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52239_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:12:38.40 -06:40:47.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 1.049 2475792906611526144 018.16028318857 -06.67982638940 13.1932 12.5455 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.049#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52241_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52241_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:12:14.28 -06:27:32.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 1.148 2475812663460892032 018.05972500712 -06.45866148249 13.2902 12.6616 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.148#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52243_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52243_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:14:41.86 -00:58:32.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 52250_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52250_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:13:26.50 -06:34:21.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 0.954 2475771607869384576 018.36066505827 -06.57259670842 13.3936 12.8010 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.954#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52261_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52261_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:12:07.34 -06:13:09.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 1.513 2475842801247249792 018.03088704253 -06.21887420622 13.5748 12.9679 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.513#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52262_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52262_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:12:10.19 -06:47:34.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 1.158 2475738828678942208 018.04261955816 -06.79255418673 13.4996 12.9721 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.158#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52267_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52267_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:12:04.39 -06:42:55.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 0.663 2475787378989254784 018.01819504763 -06.71546284902 13.5189 12.8052 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.663#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52277_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52277_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:12:57.41 -06:41:33.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 0.710 2475746490900612608 018.23931823942 -06.69271982183 13.3523 12.5134 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.710#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52278_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52278_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:12:13.45 -06:56:30.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 0.248 2475732265968915072 018.05609871344 -06.94184954638 13.6515 13.1333 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.248#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52282_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52282_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:13:08.60 -06:57:38.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 0.999 2475720274420243328 018.28584011618 -06.96050024082 13.6206 13.0294 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.999#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52283_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52283_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:12:04.01 -06:16:18.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 1.119 2475842354570651520 018.01694445995 -06.27203703796 13.9130 13.2924 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.119#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52285_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52285_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:22:35.22 -00:25:35.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 52286_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52286_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:32:56.32 +00:06:03.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 4.286 2510018955533104896 023.23372577839 +00.10024278658 13.7422 12.7794 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.286#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52294_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52294_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:12:32.34 -06:11:42.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 1.823 2475843832039425152 018.13508529648 -06.19470205742 13.5087 12.9422 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.823#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52298_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52298_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:13:16.59 -06:43:24.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 1.508 2475743261085218304 018.31895015812 -06.72300773196 13.7854 13.0903 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.508#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52300_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52300_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:24:19.59 -01:44:42.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52308_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52308_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:13:35.60 -06:53:20.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 1.594 2475727180727688192 018.39876849235 -06.88915199799 13.7449 13.1044 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.594#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52313_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
Preparing report for the candidate 52313_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52315_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52315_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:12:33.86 -06:34:23.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 0.911 2475795934564121984 018.14102604565 -06.57332997772 13.9230 13.2782 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.911#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52317_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52317_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:39:55.22 -02:28:24.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.05, MAG_FAINT_SEARCH_LIMIT=15.03)GAIADR2_OUTPUT=# 1.468 2484481492307817856 024.97972330510 -02.47336363883 14.2865 13.8586 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.468#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52320_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52320_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:54:34.66 -00:44:39.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)GAIADR2_OUTPUT=# 1.641 2506150564388805248 028.64396758815 -00.74446761168 14.5850 14.0667 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.641#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52322_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 52322_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 01:12:16.30 -06:22:08.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 1.748 2475837441128066944 018.06826456407 -06.36854796912 13.9239 13.3286 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.748#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52328_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
Preparing report for the candidate 52328_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02108_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 02108_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks
**** FOUND 02:01:47.52 +02:38:14.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 00890_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070
The candidate 00890_fd_Cet-03-Q1b1x1_2026-02-11_21-07-58_20.00sec_-15.00C_LIGHT_0070 did not pass the final checks