This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX
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,2461121.7520,14.43,0.05,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 20260322.2520 14.43CV 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-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:18:47.23 +33:28:55.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20_00sec_-14_90C_LIGHT_0658_fits__*pix.png resample_wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20_00sec_-14_90C_LIGHT_0125_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20_00sec_-14_90C_LIGHT_0658_fits__*pix.png resample_wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20_00sec_-14_90C_LIGHT_0124_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20_00sec_-14_90C_LIGHT_0658_fits__*pix.png resample_wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20_00sec_-14_90C_LIGHT_0125_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20_00sec_-14_90C_LIGHT_0658_fits__*pix.png resample_wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20_00sec_-14_90C_LIGHT_0124_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,2461121.7520,14.84,0.05,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 20260322.2520 14.84CV 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-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:34:02.81 +26:35:58.6 ;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-01-Q2b1x1_2025-12-23_05-58-58_20_00sec_-14_90C_LIGHT_0658_fits__*pix.png resample_wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20_00sec_-14_90C_LIGHT_0125_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20_00sec_-14_90C_LIGHT_0658_fits__*pix.png resample_wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20_00sec_-14_90C_LIGHT_0124_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20_00sec_-14_90C_LIGHT_0658_fits__*pix.png resample_wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20_00sec_-14_90C_LIGHT_0125_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20_00sec_-14_90C_LIGHT_0658_fits__*pix.png resample_wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20_00sec_-14_90C_LIGHT_0124_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
target,2461121.7520,14.87,0.05,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
target 20260322.2520 14.87CV 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-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:13:16.12 +31:21:27.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20_00sec_-14_90C_LIGHT_0658_fits__*pix.png resample_wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20_00sec_-14_90C_LIGHT_0125_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20_00sec_-14_90C_LIGHT_0658_fits__*pix.png resample_wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20_00sec_-14_90C_LIGHT_0124_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20_00sec_-14_90C_LIGHT_0658_fits__*pix.png resample_wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20_00sec_-14_90C_LIGHT_0125_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20_00sec_-14_90C_LIGHT_0658_fits__*pix.png resample_wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20_00sec_-14_90C_LIGHT_0124_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.99940255 23.12.2025 11:58:58.380 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits
First image: 2461032.99940255 23.12.2025 11:58:58.380 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits
Last image: 2461121.75227716 22.03.2026 06:03:06.747 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 15
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.48
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: 10 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): 8290
Objects passed selection criteria: 8289
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 8014
Average stars matched: 7740.25 (96.5841 %)
Memory usage VmPeak: 114512 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 Sun Mar 22 02:07:48 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.99940255 23.12.2025 11:58:58.380 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits
First image: 2461032.99940255 23.12.2025 11:58:58.380 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits
Last image: 2461121.75227716 22.03.2026 06:03:06.747 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 74
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.21
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: 22 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): 44947
Objects passed selection criteria: 44832
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 43280
Average stars matched: 41783.2 (96.5417 %)
Memory usage VmPeak: 147152 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 Sun Mar 22 02:09:01 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-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits
SExtractor catalog cache: saved Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits.cat to cache
SExtractor catalog cache: saved Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.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-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.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: 2461121.75166264
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-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits exists and is non-empty
Saving wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits to local_wcs_cache/
'wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits' -> 'local_wcs_cache/wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits'
wcs_Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits exists and is non-empty
Saving wcs_Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits to local_wcs_cache/
'wcs_Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits' -> 'local_wcs_cache/wcs_Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits'
wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits exists and is non-empty
Saving wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits to local_wcs_cache/
'wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits' -> 'local_wcs_cache/wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits'
wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits exists and is non-empty
Saving wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits to local_wcs_cache/
'wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits' -> 'local_wcs_cache/wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:59:59.518 +29:59:58.37
Second-epoch image center 09:00:05.717 +29:59:23.09
Angular distance between the image centers 0.02 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:59:59.518 +29:59:58.37
Second-epoch image center 09:00:08.163 +29:59:22.96
Angular distance between the image centers 0.03 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 09:00:05.717 +29:59:23.09
Second-epoch second image center 09:00:08.163 +29:59:22.96
Angular distance between the image centers 0.00883 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-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits &> /tmp/tmp.66J2bpOnsu
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits &> /tmp/tmp.IMDw3Fg56l
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits &> /tmp/tmp.k84yUXSnSw
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits &> /tmp/tmp.uerEeDqOcz
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.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-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits and wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.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-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits and wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits.cat
Found non-empty wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits and wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits.cat
The reference image (wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits) and catalog (wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits.cat) found
'wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.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 5293 out of 9643 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.928697
a=0.000000 b=1.000000 c=22.928697
From vast_summary.log: estimated ref. image limiting mag.: -7.48
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.45
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.45
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 12 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits
2.1 pix Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits
2.4 pix fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits
2.4 pix fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits
Limiting magnitude estimates:
15.5 mag. Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits
15.4 mag. Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits
15.3 mag. fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits
15.3 mag. fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits
All-image limiting magnitude estimate: 15.3 (SNR ) 12.4 (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.66J2bpOnsu (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.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-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits' -> 'wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits
WCS_IMAGE_NAME=wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits
WCS-calibrated image found: wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits
Checking if the catalog wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits.cat corresponding to the image wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits alredy exist and is non-empty...
Catalog wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits.cat corresponding to the image wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits
WCS catalog name: wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=752, passed=9643
Got 9643 stars (including 8876 good ones) from the SExtractor catalog wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits.cat
util/solve_plate_with_UCAC5 got 9643 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits -region wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.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.IMDw3Fg56l (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.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-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits' -> 'wcs_Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits
WCS_IMAGE_NAME=wcs_Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits
WCS-calibrated image found: wcs_Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits
Checking if the catalog wcs_Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits.cat corresponding to the image wcs_Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits alredy exist and is non-empty...
Catalog wcs_Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits.cat corresponding to the image wcs_Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits
WCS catalog name: wcs_Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=779, passed=9654
Got 9654 stars (including 8863 good ones) from the SExtractor catalog wcs_Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits.cat
util/solve_plate_with_UCAC5 got 9654 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.32"
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits -region wcs_Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.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.k84yUXSnSw (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_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.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_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits
WCS-calibrated image found: wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits
Checking if the catalog wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits.cat corresponding to the image wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits.cat corresponding to the image wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits
WCS catalog name: wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=649, passed=10164
Got 10164 stars (including 9506 good ones) from the SExtractor catalog wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits.cat
util/solve_plate_with_UCAC5 got 10164 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
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: 0.41"
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_fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits -region wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.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.uerEeDqOcz (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_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.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_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits
WCS-calibrated image found: wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits
Checking if the catalog wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits.cat corresponding to the image wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits.cat corresponding to the image wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits
WCS catalog name: wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=646, passed=10125
Got 10125 stars (including 9472 good ones) from the SExtractor catalog wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits.cat
util/solve_plate_with_UCAC5 got 10125 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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 958 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: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
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 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.41"
Estimated accuracy of the plate solution: 0.41"
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_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits -region wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.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-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits'
Saving fully-calibrated image wcs_Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/wcs_Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits'
Saving fully-calibrated image wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits'
Saving fully-calibrated image wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits'
Preparing the HTML report for the field Cnc-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20420.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20422.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20462.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 4s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20420_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125
The candidate 20420_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125 did not pass the final checks
**** FOUND 09:27:41.78 +31:47:44.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 0.725 700894510443458688 141.92425512403 +31.79541676178 12.3551 11.9384 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.725#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20422_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125
The candidate 20422_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125 did not pass the final checks
**** FOUND 08:37:28.47 +29:06:30.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.03, MAG_FAINT_SEARCH_LIMIT=12.01)GAIADR2_OUTPUT=# 1.381 704701058356382976 129.36883379438 +29.10872631068 11.2851 10.8828 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.381#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20437_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125
The candidate 20437_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125 did not pass the final checks
**** FOUND 09:25:16.98 +29:58:47.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20447_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125
The candidate 20447_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125 did not pass the final checks
**** FOUND 09:00:47.47 +29:04:21.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20450_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125
The candidate 20450_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125 did not pass the final checks
**** FOUND 09:30:06.63 +30:01:45.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20454_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125
The candidate 20454_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125 did not pass the final checks
**** FOUND 09:10:23.39 +31:20:52.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20455_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125
The candidate 20455_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125 did not pass the final checks
**** FOUND 08:58:24.47 +30:20:51.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20459_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125
The candidate 20459_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125 did not pass the final checks
**** FOUND 09:04:41.06 +31:49:06.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20461_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125
The candidate 20461_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125 did not pass the final checks
**** FOUND 09:02:02.85 +30:55:32.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20462_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125
The candidate 20462_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125 did not pass the final checks
**** FOUND 08:46:38.92 +28:49:55.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 0.855 705209273246500736 131.66217968929 +28.83232052780 12.5266 11.9204 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.855#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20463_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125
The candidate 20463_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125 did not pass the final checks
**** FOUND 08:59:04.03 +31:35:07.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20464_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125
The candidate 20464_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125 did not pass the final checks
**** FOUND 09:00:19.10 +29:16:32.1 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 4s
Prepared the HTML report for the field Cnc-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits
SExtractor catalog cache: saved Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits.cat to cache
SExtractor catalog cache: saved Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.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-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits
Creating symlink local_wcs_cache/wcs_Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.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-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits exists and is non-empty
wcs_Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits exists and is non-empty
wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits exists and is non-empty
wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:59:59.518 +29:59:58.37
Second-epoch image center 09:00:05.717 +29:59:23.09
Angular distance between the image centers 0.02 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:59:59.518 +29:59:58.37
Second-epoch image center 09:00:08.163 +29:59:22.96
Angular distance between the image centers 0.03 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 09:00:05.717 +29:59:23.09
Second-epoch second image center 09:00:08.163 +29:59:22.96
Angular distance between the image centers 0.00883 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-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits &> /tmp/tmp.W8OzgmaE4Y
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits &> /tmp/tmp.eTf39bWDNl
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits &> /tmp/tmp.gZzxPk5q68
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits &> /tmp/tmp.rYBAypa6X4
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.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-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits and wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.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-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits and wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits.cat
Found non-empty wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits and wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits.cat
The reference image (wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits) and catalog (wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits.cat) found
'wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.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 5342 out of 54114 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.827935
a=0.000000 b=1.000000 c=22.827935
From vast_summary.log: estimated ref. image limiting mag.: -7.21
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.62
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.62
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 21 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits
2.0 pix Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits
2.4 pix fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits
2.4 pix fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits
Limiting magnitude estimates:
15.6 mag. Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits
15.6 mag. Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits
15.4 mag. fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits
15.4 mag. fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits
All-image limiting magnitude estimate: 15.4 (SNR ) 14.7 (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.W8OzgmaE4Y (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.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-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits' -> 'wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits
WCS_IMAGE_NAME=wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits
WCS-calibrated image found: wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits
Checking if the catalog wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits.cat corresponding to the image wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits alredy exist and is non-empty...
Catalog wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits.cat corresponding to the image wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits
WCS catalog name: wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits.cat
SExtractor catalog parsing summary: zero_flux=2, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=30, blended=2874, passed=54082
Got 54082 stars (including 51106 good ones) from the SExtractor catalog wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits.cat
util/solve_plate_with_UCAC5 got 54082 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.34"
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_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits -region wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.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.eTf39bWDNl (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.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-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits' -> 'wcs_Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits
WCS_IMAGE_NAME=wcs_Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits
WCS-calibrated image found: wcs_Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits
Checking if the catalog wcs_Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits.cat corresponding to the image wcs_Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits alredy exist and is non-empty...
Catalog wcs_Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits.cat corresponding to the image wcs_Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits
WCS catalog name: wcs_Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=27, blended=2821, passed=53970
Got 53970 stars (including 51052 good ones) from the SExtractor catalog wcs_Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits.cat
util/solve_plate_with_UCAC5 got 53970 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.34"
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-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits -region wcs_Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.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.gZzxPk5q68 (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_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.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_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits
WCS-calibrated image found: wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits
Checking if the catalog wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits.cat corresponding to the image wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits.cat corresponding to the image wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits
WCS catalog name: wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=2684, passed=48496
Got 48496 stars (including 45749 good ones) from the SExtractor catalog wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits.cat
util/solve_plate_with_UCAC5 got 48496 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
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: 0.41"
Estimated accuracy of the plate solution: 0.42"
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-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits -region wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.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.rYBAypa6X4 (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_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.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_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits
WCS-calibrated image found: wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits
Checking if the catalog wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits.cat corresponding to the image wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits.cat corresponding to the image wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits
WCS catalog name: wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=23, blended=2742, passed=48559
Got 48559 stars (including 45756 good ones) from the SExtractor catalog wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits.cat
util/solve_plate_with_UCAC5 got 48559 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
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: 0.41"
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 954 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-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits -region wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.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-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.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_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/wcs_Cnc-01-Q2b1x1_2025-12-23_05-58-58_20.00sec_-14.90C_LIGHT_0658.fits
Saving fully-calibrated image wcs_Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.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_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/wcs_Cnc-01-Q2b1x1_2025-12-23_05-59-51_20.00sec_-15.00C_LIGHT_0659.fits
Saving fully-calibrated image wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.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_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-02-13_20.00sec_-14.90C_LIGHT_0124.fits
Saving fully-calibrated image wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.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_2026-03-22_CI_Cnc-01-Q2b1x1_015906_TTUQ2b1x1_3440_LGtgp7nX/wcs_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125.fits
Preparing the HTML report for the field Cnc-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out67315.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67317.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67321.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67724.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67738.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67740.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67743.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67829.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67832.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67874.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67899.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out67687.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67762.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67931.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 19s
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 67315_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125
The candidate 67315_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125 did not pass the final checks
**** FOUND 08:46:17.05 +31:43:57.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.72, MAG_FAINT_SEARCH_LIMIT=15.70)GAIADR2_OUTPUT=# 1.240 706902933468914816 131.57137758281 +31.73280351923 14.9772 14.5381 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.240#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67317_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125
The candidate 67317_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125 did not pass the final checks
**** FOUND 08:55:28.72 +33:23:53.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.79, MAG_FAINT_SEARCH_LIMIT=15.77)GAIADR2_OUTPUT=# 0.909 713158536155885184 133.86979176963 +33.39782569937 14.7075 14.2013 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.909#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67321_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125
The candidate 67321_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125 did not pass the final checks
**** FOUND 08:54:05.40 +34:08:19.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)GAIADR2_OUTPUT=# 0.291 713256835070558464 133.52250725717 +34.13853056209 14.3263 13.6890 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.291#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67323_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125
The candidate 67323_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125 did not pass the final checks
**** FOUND 08:48:09.36 +33:19:08.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67476_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125
The candidate 67476_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125 did not pass the final checks
**** FOUND 08:33:17.14 +31:02:20.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67479_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125
The candidate 67479_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125 did not pass the final checks
**** FOUND 08:43:01.79 +33:36:28.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67536_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125
The candidate 67536_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125 did not pass the final checks
**** FOUND 08:33:07.90 +31:29:37.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67547_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125
The candidate 67547_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125 did not pass the final checks
**** FOUND 08:38:03.94 +28:36:28.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67687_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125
Preparing report for the candidate 67687_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125
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Considering the candidate 67724_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125
The candidate 67724_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125 did not pass the final checks
**** FOUND 08:37:41.59 +26:02:57.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.72, MAG_FAINT_SEARCH_LIMIT=15.70)GAIADR2_OUTPUT=# 2.518 702984755064734848 129.42406627138 +26.04940212718 14.9076 14.2439 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.518#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67738_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125
The candidate 67738_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125 did not pass the final checks
**** FOUND 08:33:13.25 +29:28:10.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.79, MAG_FAINT_SEARCH_LIMIT=15.77)GAIADR2_OUTPUT=# 0.481 707691798702348416 128.30526652542 +29.46954315423 14.8323 14.3692 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.481#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67740_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125
The candidate 67740_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125 did not pass the final checks
**** FOUND 08:34:46.90 +26:16:38.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.81, MAG_FAINT_SEARCH_LIMIT=15.79)
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Considering the candidate 67743_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125
The candidate 67743_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125 did not pass the final checks
**** FOUND 08:31:53.27 +31:18:01.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.90, MAG_FAINT_SEARCH_LIMIT=15.88)GAIADR2_OUTPUT=# 0.725 708189740030197760 127.97188828359 +31.30066455985 14.8526 14.3076 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.725#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67762_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125
Preparing report for the candidate 67762_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125
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Considering the candidate 67829_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125
The candidate 67829_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125 did not pass the final checks
**** FOUND 08:34:07.44 +29:24:05.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.93, MAG_FAINT_SEARCH_LIMIT=15.91)GAIADR2_OUTPUT=# 1.495 707679532275816320 128.53065703868 +29.40187160550 14.9580 14.4035 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.495#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67832_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125
The candidate 67832_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125 did not pass the final checks
**** FOUND 08:38:30.35 +30:22:15.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.97, MAG_FAINT_SEARCH_LIMIT=15.95)GAIADR2_OUTPUT=# 1.254 709329658711437184 129.62685079597 +30.37102673281 14.7019 13.8049 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.254#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67874_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125
The candidate 67874_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125 did not pass the final checks
**** FOUND 08:38:28.58 +26:25:29.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.88, MAG_FAINT_SEARCH_LIMIT=15.86)GAIADR2_OUTPUT=# 0.754 703024578001473920 129.61917882016 +26.42505233344 15.0558 14.5315 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.754#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67899_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125
The candidate 67899_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125 did not pass the final checks
**** FOUND 08:32:59.09 +27:04:07.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.98, MAG_FAINT_SEARCH_LIMIT=15.96)GAIADR2_OUTPUT=# 0.770 703903156511364736 128.24597949936 +27.06857391861 15.0213 14.4461 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.770#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67931_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125
Preparing report for the candidate 67931_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125
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Considering the candidate 48812_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125
The candidate 48812_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125 did not pass the final checks
Rejecting candidate due to large distance (31.9") between the two second-epoch detections
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Considering the candidate 25383_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125
The candidate 25383_fd_Cnc-01-Q2b1x1_2026-03-22_01-03-06_20.00sec_-14.90C_LIGHT_0125 did not pass the final checks