This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb
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!
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,2461124.7627,13.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260325.2627 13.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:21:36.41 +20:06:28.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20_00sec_-14_90C_LIGHT_0144_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20_00sec_-15_00C_LIGHT_0043_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20_00sec_-14_90C_LIGHT_0144_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20_00sec_-14_90C_LIGHT_0042_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20_00sec_-14_90C_LIGHT_0144_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20_00sec_-14_90C_LIGHT_0144_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20_00sec_-14_90C_LIGHT_0042_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!
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,2461124.7627,14.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260325.2627 14.05CV 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/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:01:51.61 +22:28:25.6 ;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_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20_00sec_-14_90C_LIGHT_0144_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20_00sec_-15_00C_LIGHT_0043_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20_00sec_-14_90C_LIGHT_0144_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20_00sec_-14_90C_LIGHT_0042_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20_00sec_-14_90C_LIGHT_0144_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20_00sec_-14_90C_LIGHT_0144_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20_00sec_-14_90C_LIGHT_0042_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!
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,2461124.7627,14.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260325.2627 14.24CV 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/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:00:49.86 +22:03:41.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20_00sec_-14_90C_LIGHT_0144_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20_00sec_-15_00C_LIGHT_0043_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20_00sec_-14_90C_LIGHT_0144_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20_00sec_-14_90C_LIGHT_0042_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20_00sec_-14_90C_LIGHT_0144_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20_00sec_-14_90C_LIGHT_0144_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 25.2627* 09 22 58.35 +25 28 10.4 14.3 U Leo 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,2461124.7627,14.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260325.2627 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/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:22:58.35 +25:28:10.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20_00sec_-14_90C_LIGHT_0144_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20_00sec_-15_00C_LIGHT_0043_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20_00sec_-14_90C_LIGHT_0144_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20_00sec_-14_90C_LIGHT_0042_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20_00sec_-14_90C_LIGHT_0144_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20_00sec_-14_90C_LIGHT_0144_fits__*pix.png resample_wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20_00sec_-14_90C_LIGHT_0042_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: 2461119.67641736 20.03.2026 04:13:52.460 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
First image: 2461119.67641736 20.03.2026 04:13:52.460 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
Last image: 2461124.76297448 25.03.2026 06:18:30.995 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.60
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): 7126
Objects passed selection criteria: 7109
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 5939.25
Average stars matched: 5869.5 (98.8256 %)
Memory usage VmPeak: 113880 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Mar 25 01:38:06 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461119.67641736 20.03.2026 04:13:52.460 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
First image: 2461119.67641736 20.03.2026 04:13:52.460 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
Last image: 2461124.76297448 25.03.2026 06:18:30.995 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 50
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.32
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: 15 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): 37448
Objects passed selection criteria: 37378
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: 33783.8
Average stars matched: 32716.8 (96.8417 %)
Memory usage VmPeak: 141988 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Mar 25 01:38:49 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits
SExtractor catalog cache: saved Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat to cache
SExtractor catalog cache: saved Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.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/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.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: 2461124.76239994
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_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits exists and is non-empty
Saving wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits to local_wcs_cache/
'wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits' -> 'local_wcs_cache/wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits'
wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits exists and is non-empty
Saving wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits to local_wcs_cache/
'wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits' -> 'local_wcs_cache/wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits'
wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits exists and is non-empty
Saving wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits to local_wcs_cache/
'wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits' -> 'local_wcs_cache/wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits'
wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits exists and is non-empty
Saving wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits to local_wcs_cache/
'wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits' -> 'local_wcs_cache/wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits'
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:14:05.815 +22:02:06.51
Second-epoch image center 09:13:52.359 +22:00:02.44
Angular distance between the image centers 0.06 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 09:14:05.815 +22:02:06.51
Second-epoch image center 09:13:53.202 +21:59:21.98
Angular distance between the image centers 0.07 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 09:13:52.359 +22:00:02.44
Second-epoch second image center 09:13:53.202 +21:59:21.98
Angular distance between the image centers 0.01170 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/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits &> /tmp/tmp.2nGOez2uau
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits &> /tmp/tmp.Ax00nSTTK4
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits &> /tmp/tmp.kgu0vLWjgD
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits &> /tmp/tmp.8kbUb1PWf6
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.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_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits and wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.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_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits and wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat
Found non-empty wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits and wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat
The reference image (wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits) and catalog (wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat) found
'wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.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 4760 out of 9535 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.916671
a=0.000000 b=1.000000 c=22.916671
From vast_summary.log: estimated ref. image limiting mag.: -7.60
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.32
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.32
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.5 pix Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
2.3 pix Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
2.4 pix fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits
2.4 pix fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits
Limiting magnitude estimates:
15.3 mag. Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
15.4 mag. Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
14.6 mag. fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits
14.7 mag. fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 11.7 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.2nGOez2uau (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_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits' -> 'wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
WCS_IMAGE_NAME=wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
WCS-calibrated image found: wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
Checking if the catalog wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat corresponding to the image wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits alredy exist and is non-empty...
Catalog wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat corresponding to the image wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
WCS catalog name: wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=608, passed=9535
Got 9535 stars (including 8921 good ones) from the SExtractor catalog wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat
util/solve_plate_with_UCAC5 got 9535 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 956 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: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
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 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.43"
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits -region wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.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.Ax00nSTTK4 (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_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits' -> 'wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
WCS_IMAGE_NAME=wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
WCS-calibrated image found: wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
Checking if the catalog wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits.cat corresponding to the image wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits alredy exist and is non-empty...
Catalog wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits.cat corresponding to the image wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
WCS catalog name: wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=669, passed=9214
Got 9214 stars (including 8536 good ones) from the SExtractor catalog wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits.cat
util/solve_plate_with_UCAC5 got 9214 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 956 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: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.46"
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 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.46"
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits -region wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.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.kgu0vLWjgD (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits
WCS-calibrated image found: wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits
Checking if the catalog wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits.cat corresponding to the image wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits.cat corresponding to the image wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits
WCS catalog name: wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=346, passed=5635
Got 5635 stars (including 5283 good ones) from the SExtractor catalog wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits.cat
util/solve_plate_with_UCAC5 got 5635 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 954 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: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.47"
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 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.47"
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 953 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits -region wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.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.8kbUb1PWf6 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits
WCS-calibrated image found: wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits
Checking if the catalog wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits.cat corresponding to the image wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits.cat corresponding to the image wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits
WCS catalog name: wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=348, passed=5691
Got 5691 stars (including 5335 good ones) from the SExtractor catalog wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits.cat
util/solve_plate_with_UCAC5 got 5691 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 954 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: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.48"
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 953 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits -region wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.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_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits'
Saving fully-calibrated image wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits'
Saving fully-calibrated image wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits'
Saving fully-calibrated image wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits'
Preparing the HTML report for the field Cnc-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Cnc-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits
SExtractor catalog cache: saved Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat to cache
SExtractor catalog cache: saved Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
Creating symlink local_wcs_cache/wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.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_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits exists and is non-empty
wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits exists and is non-empty
wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits exists and is non-empty
wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits exists and is non-empty
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:14:05.815 +22:02:06.51
Second-epoch image center 09:13:52.359 +22:00:02.44
Angular distance between the image centers 0.06 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 09:14:05.815 +22:02:06.51
Second-epoch image center 09:13:53.202 +21:59:21.98
Angular distance between the image centers 0.07 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 09:13:52.359 +22:00:02.44
Second-epoch second image center 09:13:53.202 +21:59:21.98
Angular distance between the image centers 0.01170 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/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits &> /tmp/tmp.k3ktCUlCGA
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits &> /tmp/tmp.SOK6oLXY7c
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits &> /tmp/tmp.qVOcrGLkJ2
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits &> /tmp/tmp.9NJcyaE5Fz
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.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_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits and wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.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_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits and wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat
Found non-empty wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits and wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat
The reference image (wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits) and catalog (wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat) found
'wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.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 4779 out of 46595 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.803264
a=0.000000 b=1.000000 c=22.803264
From vast_summary.log: estimated ref. image limiting mag.: -7.32
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.48
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.48
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 34 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
2.1 pix Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
2.2 pix fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits
2.2 pix fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits
Limiting magnitude estimates:
15.5 mag. Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
15.5 mag. Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
14.8 mag. fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits
14.9 mag. fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 14.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.k3ktCUlCGA (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_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits' -> 'wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
WCS_IMAGE_NAME=wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
WCS-calibrated image found: wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
Checking if the catalog wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat corresponding to the image wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits alredy exist and is non-empty...
Catalog wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat corresponding to the image wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
WCS catalog name: wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=22, blended=2637, passed=46573
Got 46573 stars (including 43885 good ones) from the SExtractor catalog wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat
util/solve_plate_with_UCAC5 got 46573 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 957 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: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.44"
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 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.44"
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits -region wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.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.SOK6oLXY7c (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_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits' -> 'wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
WCS_IMAGE_NAME=wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
WCS-calibrated image found: wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
Checking if the catalog wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits.cat corresponding to the image wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits alredy exist and is non-empty...
Catalog wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits.cat corresponding to the image wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
WCS catalog name: wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=2639, passed=48659
Got 48659 stars (including 45945 good ones) from the SExtractor catalog wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits.cat
util/solve_plate_with_UCAC5 got 48659 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 956 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: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.46"
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 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.46"
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits -region wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.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.qVOcrGLkJ2 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits
WCS-calibrated image found: wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits
Checking if the catalog wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits.cat corresponding to the image wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits.cat corresponding to the image wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits
WCS catalog name: wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=1266, passed=31731
Got 31731 stars (including 30439 good ones) from the SExtractor catalog wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits.cat
util/solve_plate_with_UCAC5 got 31731 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.47"
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 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.47"
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 952 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits -region wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.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.9NJcyaE5Fz (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits
WCS-calibrated image found: wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits
Checking if the catalog wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits.cat corresponding to the image wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits.cat corresponding to the image wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits
WCS catalog name: wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=1253, passed=32422
Got 32422 stars (including 31132 good ones) from the SExtractor catalog wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits.cat
util/solve_plate_with_UCAC5 got 32422 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 955 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: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.48"
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 955 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits -region wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.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_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
Saving fully-calibrated image wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
Saving fully-calibrated image wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-17-41_20.00sec_-14.90C_LIGHT_0042.fits
Saving fully-calibrated image wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-03-Q2b1x1_013553_TTUQ2b1x1_1307_JRIgvcUb/wcs_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043.fits
Preparing the HTML report for the field Cnc-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out53879.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53882.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53884.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53886.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53887.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53888.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53889.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53995.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53996.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53999.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54003.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54021.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54034.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54044.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54045.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54047.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54051.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54054.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54059.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54060.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54065.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54067.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54086.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54093.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54103.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54104.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54135.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54142.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out54037.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54064.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54112.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54122.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 53879_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043
The candidate 53879_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 09:34:49.73 +24:26:58.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)GAIADR2_OUTPUT=# 2.257 644934453831023744 143.70688041139 +24.44889319725 13.7096 13.0488 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.257#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53882_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043
The candidate 53882_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 09:28:01.26 +23:18:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 1.329 639135805600514816 142.00550691518 +23.30333944343 13.6351 13.1504 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.329#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53884_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043
The candidate 53884_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 09:17:55.47 +20:03:06.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 0.487 636047788538356992 139.48104816629 +20.05174664867 13.2040 12.8217 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.487#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53886_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043
The candidate 53886_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 09:16:17.74 +18:22:03.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 1.955 635576308504216704 139.07381449178 +18.36803426495 13.0933 12.5340 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.955#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53887_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043
The candidate 53887_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 09:18:15.52 +18:23:11.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)GAIADR2_OUTPUT=# 1.548 632577695481696000 139.56466890030 +18.38704117366 12.4485 12.0194 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.548#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53888_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043
The candidate 53888_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 09:25:14.57 +18:45:01.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 1.641 632473310597037952 141.31038594165 +18.75018926231 12.5248 12.0021 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#
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Considering the candidate 53889_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043
The candidate 53889_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 09:24:09.30 +19:57:42.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.21, MAG_FAINT_SEARCH_LIMIT=12.19)GAIADR2_OUTPUT=# 3.030 637298074993529600 141.03845984964 +19.96251838128 11.3344 10.6640 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.030#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53995_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043
The candidate 53995_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 09:42:15.78 +24:29:19.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 1.992 644751561238913280 145.56551707203 +24.48826662228 13.3509 12.7256 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.992#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53996_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043
The candidate 53996_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 09:16:16.49 +23:25:02.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 1.295 686991288989860480 139.06888883901 +23.41756928563 13.3003 12.7499 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.295#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53999_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043
The candidate 53999_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 09:10:55.87 +18:54:57.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 0.371 635536760444995456 137.73276603982 +18.91601691418 13.3386 12.8745 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.371#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54003_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043
The candidate 54003_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 09:20:35.06 +22:39:16.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)
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Considering the candidate 54021_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043
The candidate 54021_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 09:32:55.33 +23:22:07.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 1.680 644347177183461504 143.23096775425 +23.36897661101 13.8093 13.2751 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.680#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54034_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043
The candidate 54034_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 09:12:47.99 +20:01:54.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 0.557 636739037754821632 138.19982183919 +20.03178076991 13.6764 13.1442 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.557#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54037_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043
Preparing report for the candidate 54037_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043
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Considering the candidate 54044_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043
The candidate 54044_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 09:35:49.65 +18:04:43.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 2.758 632975722985984512 143.95630876369 +18.07932305537 13.7164 13.1032 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.758#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54045_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043
The candidate 54045_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 09:32:04.96 +25:26:05.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 2.131 645805580573178624 143.02009704342 +25.43512629638 13.6523 12.5445 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.131#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54047_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043
The candidate 54047_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 09:22:54.97 +21:56:34.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 2.459 638193180537721216 140.72849747209 +21.94256759242 13.9202 13.4067 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.459#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54051_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043
The candidate 54051_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 09:36:07.05 +24:56:55.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 0.462 644985757215805952 144.02949550048 +24.94887264210 13.9324 13.4614 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#
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Considering the candidate 54054_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043
The candidate 54054_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 09:17:41.83 +20:48:59.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 1.491 637636243538535936 139.42386960748 +20.81648512204 14.2658 13.7938 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.491#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54059_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043
The candidate 54059_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 09:35:58.17 +23:11:20.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 1.717 644234786478841856 143.99197061388 +23.18924307735 13.6749 12.8191 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.717#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54060_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043
The candidate 54060_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 09:29:04.54 +17:50:58.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.03, MAG_FAINT_SEARCH_LIMIT=15.01)GAIADR2_OUTPUT=# 3.231 631605937656173440 142.26900092140 +17.85044941994 13.9623 13.5288 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.231#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54064_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043
Preparing report for the candidate 54064_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043
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Considering the candidate 54065_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043
The candidate 54065_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 09:06:05.08 +24:46:16.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 0.717 688349877341041408 136.52100379491 +24.77124465298 13.9279 13.3864 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.717#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54067_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043
The candidate 54067_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 09:24:28.57 +19:04:50.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 3.717 634182024680964096 141.11871292947 +19.08167895246 14.1028 13.8959 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.717#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54071_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043
The candidate 54071_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 09:44:01.81 +25:18:51.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54080_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043
The candidate 54080_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 09:38:35.93 +19:25:43.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54086_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043
The candidate 54086_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 09:17:52.21 +25:59:42.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 1.352 693928004770019840 139.46754905120 +25.99479109754 14.3975 13.9619 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.352#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54093_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043
The candidate 54093_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 08:55:05.23 +19:52:13.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 0.959 660779554555183360 133.77171388801 +19.87072836977 14.1115 13.4821 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.959#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54103_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043
The candidate 54103_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 08:57:30.08 +21:22:13.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.19, MAG_FAINT_SEARCH_LIMIT=15.17)GAIADR2_OUTPUT=# 1.118 685062234494498304 134.37532684805 +21.37083827636 14.1283 13.5818 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.118#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54104_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043
The candidate 54104_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 09:11:14.03 +18:40:42.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 2.047 635461272099853952 137.80797999455 +18.67807329390 14.1609 13.6101 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.047#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54112_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043
Preparing report for the candidate 54112_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043
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Considering the candidate 54122_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043
Preparing report for the candidate 54122_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043
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Considering the candidate 54135_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043
The candidate 54135_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 09:31:11.71 +21:09:23.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 1.002 634858804152156928 142.79890587499 +21.15684036404 14.0129 13.2245 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.002#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54142_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043
The candidate 54142_fd_Cnc-03-Q2b1x1_2026-03-25_01-18-30_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks