This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw
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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461147.7326,14.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260417.2326 14.30CV 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
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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461147.7326,14.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260417.2326 14.90CV 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461082.76664567 11.02.2026 06:23:48.186 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits
First image: 2461082.76664567 11.02.2026 06:23:48.186 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits
Last image: 2461147.73290414 17.04.2026 05:35:12.918 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.56
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: 4 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): 8525
Objects passed selection criteria: 8517
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 7898
Average stars matched: 7633 (96.6447 %)
Memory usage VmPeak: 113664 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Apr 17 00:37:31 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: 2461082.76664567 11.02.2026 06:23:48.186 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits
First image: 2461082.76664567 11.02.2026 06:23:48.186 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits
Last image: 2461147.73290414 17.04.2026 05:35:12.918 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 59
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.27
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: 14 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): 51045
Objects passed selection criteria: 50904
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 47631
Average stars matched: 45459.5 (95.441 %)
Memory usage VmPeak: 147908 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Apr 17 00:38:29 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/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits
SExtractor catalog cache: saved Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits.cat to cache
SExtractor catalog cache: saved Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.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-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.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: 2461147.73222606
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'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits exists and is non-empty
Saving wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits to local_wcs_cache/
'wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits' -> 'local_wcs_cache/wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits'
wcs_Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits exists and is non-empty
Saving wcs_Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits to local_wcs_cache/
'wcs_Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits' -> 'local_wcs_cache/wcs_Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits'
wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits exists and is non-empty
Saving wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits to local_wcs_cache/
'wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits' -> 'local_wcs_cache/wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits'
wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits exists and is non-empty
Saving wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits to local_wcs_cache/
'wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits' -> 'local_wcs_cache/wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits (1st reference image)
verification OK: wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits
Image size: 941.6'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 08:59:59.815 +30:00:01.62 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits (1st new image)
verification OK: wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits
Image size: 941.3'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:00:05.826 +29:59:00.21 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:59:59.815 +30:00:01.62
Second-epoch image center 09:00:05.826 +29:59:00.21
Angular distance between the image centers 0.0276 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits (2nd new image)
verification OK: wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits
Image size: 941.3'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:00:06.795 +29:59:38.38 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:59:59.815 +30:00:01.62
Second-epoch image center 09:00:06.795 +29:59:38.38
Angular distance between the image centers 0.0260 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 09:00:05.826 +29:59:00.21
Second-epoch second image center 09:00:06.795 +29:59:38.38
Angular distance between the image centers 0.01116 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-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits &> /tmp/tmp.AUr93tMWK4
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits &> /tmp/tmp.B3z88Av9mD
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits &> /tmp/tmp.POVxUoUFud
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits &> /tmp/tmp.EOdJILXZwn
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.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-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits and wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.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-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits and wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits.cat
Found non-empty wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits and wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits.cat
The reference image (wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits) and catalog (wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits.cat) found
'wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits.cat' -> 'wcsmag.cat'
Read 8224 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 125.2307 to 144.3016 deg, Dec +24.1687 to +35.3629 deg
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
Tycho-2 catalog search boundaries: RA 125.2307 to 144.3016 deg, Dec 24.1687 to 35.3629 deg
Loaded 6834 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 4962 out of 5218 total matches.
Matched with Tycho-2 5218 out of 8224 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.785680
a=0.000000 b=1.000000 c=22.785680
From vast_summary.log: estimated ref. image limiting mag.: -7.56
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.23
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.23
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits
2.0 pix Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits
2.1 pix fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits
2.1 pix fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits
Limiting magnitude estimates:
15.2 mag. Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits
15.3 mag. Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits
15.1 mag. fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits
15.1 mag. fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 12.1 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.AUr93tMWK4 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.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-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits' -> 'wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits
WCS_IMAGE_NAME=wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits
WCS-calibrated image found: wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits
Checking if the catalog wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits.cat corresponding to the image wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits alredy exist and is non-empty...
Catalog wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits.cat corresponding to the image wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits
WCS catalog name: wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=633, passed=8224
Got 8224 stars (including 7580 good ones) from the SExtractor catalog wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits.cat
util/solve_plate_with_UCAC5 got 8224 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...
Searching UCAC5 zones 570 to 628 (Dec 24.2 to 35.4)
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...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 942 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 8114 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 628 (Dec 24.2 to 35.4)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 8112 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 8112 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits -region wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.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.B3z88Av9mD (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.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-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits' -> 'wcs_Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits
WCS_IMAGE_NAME=wcs_Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits
WCS-calibrated image found: wcs_Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits
Checking if the catalog wcs_Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits.cat corresponding to the image wcs_Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits alredy exist and is non-empty...
Catalog wcs_Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits.cat corresponding to the image wcs_Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits
WCS catalog name: wcs_Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=645, passed=8312
Got 8312 stars (including 7657 good ones) from the SExtractor catalog wcs_Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits.cat
util/solve_plate_with_UCAC5 got 8312 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...
Searching UCAC5 zones 570 to 628 (Dec 24.2 to 35.4)
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...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 942 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 8202 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
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...
Searching UCAC5 zones 570 to 628 (Dec 24.2 to 35.4)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 8202 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 8202 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits -region wcs_Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.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.POVxUoUFud (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_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_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_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits
WCS-calibrated image found: wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits
Checking if the catalog wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits.cat corresponding to the image wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits.cat corresponding to the image wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_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-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits
WCS catalog name: wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_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=526, passed=7687
Got 7687 stars (including 7149 good ones) from the SExtractor catalog wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits.cat
util/solve_plate_with_UCAC5 got 7687 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 629 (Dec 24.1 to 35.5)
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...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 943 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 7606 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 629 (Dec 24.1 to 35.5)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 7608 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 7608 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
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-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits -region wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.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.EOdJILXZwn (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_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.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_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits
WCS-calibrated image found: wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits
Checking if the catalog wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits.cat corresponding to the image wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits.cat corresponding to the image wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits
WCS catalog name: wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=551, passed=7566
Got 7566 stars (including 7004 good ones) from the SExtractor catalog wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits.cat
util/solve_plate_with_UCAC5 got 7566 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 629 (Dec 24.1 to 35.5)
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 943 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 7496 with non-zero local correction accuracy
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...
Searching UCAC5 zones 570 to 629 (Dec 24.1 to 35.5)
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 7496 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 7496 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 953 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits -region wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.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-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits'
Saving fully-calibrated image wcs_Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/wcs_Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits'
Saving fully-calibrated image wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits'
Saving fully-calibrated image wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits'
Preparing the HTML report for the field Cnc-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20466.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 2s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20466_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 20466_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 09:27:41.74 +31:47:44.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 1.662 700894510443458688 141.92425512403 +31.79541676178 12.3551 11.9384 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.662#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20777_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 20777_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 08:43:32.15 +26:36:57.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20788_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 20788_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 08:52:22.75 +28:13:05.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20809_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 20809_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 09:03:01.45 +28:37:06.3 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 3s
Prepared the HTML report for the field Cnc-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits
SExtractor catalog cache: saved Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits.cat to cache
SExtractor catalog cache: saved Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.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-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits
Creating symlink local_wcs_cache/wcs_Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.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-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits exists and is non-empty
wcs_Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits exists and is non-empty
wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits exists and is non-empty
wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits (1st reference image)
verification OK: wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits
Image size: 941.6'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 08:59:59.815 +30:00:01.62 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits (1st new image)
verification OK: wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits
Image size: 941.3'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:00:05.826 +29:59:00.21 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:59:59.815 +30:00:01.62
Second-epoch image center 09:00:05.826 +29:59:00.21
Angular distance between the image centers 0.0276 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits (2nd new image)
verification OK: wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits
Image size: 941.3'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:00:06.795 +29:59:38.38 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:59:59.815 +30:00:01.62
Second-epoch image center 09:00:06.795 +29:59:38.38
Angular distance between the image centers 0.0260 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 09:00:05.826 +29:59:00.21
Second-epoch second image center 09:00:06.795 +29:59:38.38
Angular distance between the image centers 0.01116 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-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits &> /tmp/tmp.sImyJLVzLF
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits &> /tmp/tmp.cqoZRfZdGB
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits &> /tmp/tmp.Sds47lReJj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits &> /tmp/tmp.yEkYAspIJn
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.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-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits and wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.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-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits and wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits.cat
Found non-empty wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits and wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits.cat
The reference image (wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits) and catalog (wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits.cat) found
'wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits.cat' -> 'wcsmag.cat'
Read 48777 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 125.2025 to 144.3059 deg, Dec +24.1581 to +35.3659 deg
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
Tycho-2 catalog search boundaries: RA 125.2025 to 144.3059 deg, Dec 24.1581 to 35.3659 deg
Loaded 6852 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 4725 out of 5358 total matches.
Matched with Tycho-2 5358 out of 48777 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.655664
a=0.000000 b=1.000000 c=22.655664
From vast_summary.log: estimated ref. image limiting mag.: -7.27
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.39
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.39
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 49 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
1.9 pix Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits
1.8 pix Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits
2.0 pix fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits
1.9 pix fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits
Limiting magnitude estimates:
15.4 mag. Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits
15.4 mag. Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits
15.3 mag. fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits
15.3 mag. fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits
All-image limiting magnitude estimate: 15.3 (SNR ) 14.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.sImyJLVzLF (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.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-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits' -> 'wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits
WCS_IMAGE_NAME=wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits
WCS-calibrated image found: wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits
Checking if the catalog wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits.cat corresponding to the image wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits alredy exist and is non-empty...
Catalog wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits.cat corresponding to the image wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits
WCS catalog name: wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=2484, passed=48762
Got 48762 stars (including 46189 good ones) from the SExtractor catalog wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits.cat
util/solve_plate_with_UCAC5 got 48762 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...
Searching UCAC5 zones 570 to 628 (Dec 24.2 to 35.4)
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...
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 942 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 48364 with non-zero local correction accuracy
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...
Searching UCAC5 zones 570 to 628 (Dec 24.2 to 35.4)
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 48364 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 48364 with non-zero local correction accuracy
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-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits -region wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.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.cqoZRfZdGB (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.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-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits' -> 'wcs_Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits
WCS_IMAGE_NAME=wcs_Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits
WCS-calibrated image found: wcs_Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits
Checking if the catalog wcs_Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits.cat corresponding to the image wcs_Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits alredy exist and is non-empty...
Catalog wcs_Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits.cat corresponding to the image wcs_Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits
WCS catalog name: wcs_Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=23, blended=2620, passed=50074
Got 50074 stars (including 47363 good ones) from the SExtractor catalog wcs_Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits.cat
util/solve_plate_with_UCAC5 got 50074 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...
Searching UCAC5 zones 570 to 628 (Dec 24.2 to 35.4)
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...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 941 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 49658 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
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...
Searching UCAC5 zones 570 to 628 (Dec 24.2 to 35.4)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 49660 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 49661 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
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_Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits -region wcs_Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.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.Sds47lReJj (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_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_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_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits
WCS-calibrated image found: wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits
Checking if the catalog wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits.cat corresponding to the image wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits.cat corresponding to the image wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_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-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits
WCS catalog name: wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=2078, passed=46125
Got 46125 stars (including 43951 good ones) from the SExtractor catalog wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits.cat
util/solve_plate_with_UCAC5 got 46125 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 569 to 629 (Dec 24.0 to 35.5)
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...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 945 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 45781 with non-zero local correction accuracy
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...
Searching UCAC5 zones 569 to 629 (Dec 24.0 to 35.5)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 45780 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 45780 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
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-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits -region wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.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.yEkYAspIJn (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_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.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_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits
WCS-calibrated image found: wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits
Checking if the catalog wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits.cat corresponding to the image wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits.cat corresponding to the image wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits
WCS catalog name: wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=22, blended=2134, passed=46860
Got 46860 stars (including 44643 good ones) from the SExtractor catalog wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits.cat
util/solve_plate_with_UCAC5 got 46860 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 629 (Dec 24.0 to 35.5)
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...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 46511 with non-zero local correction accuracy
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...
Searching UCAC5 zones 570 to 629 (Dec 24.0 to 35.5)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 46513 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 46513 with non-zero local correction accuracy
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_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits -region wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.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-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.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_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits
Saving fully-calibrated image wcs_Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.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_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/wcs_Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits
Saving fully-calibrated image wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_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_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-34-14_20.00sec_-4.90C_LIGHTs_0125.fits
Saving fully-calibrated image wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.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_2026-04-17_CI_Cnc-01-Q1b1x1_003607_TTUQ1b1x1_2036117_HYNg9mqw/wcs_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126.fits
Preparing the HTML report for the field Cnc-01-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out54238.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54245.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54246.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54247.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54250.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55973.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56026.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56203.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56219.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56238.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56278.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56286.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56294.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56314.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56337.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out55786.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56178.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 54238_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 54238_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 09:17:10.01 +34:40:47.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.98, MAG_FAINT_SEARCH_LIMIT=15.96)GAIADR2_OUTPUT=# 3.752 714410605021912960 139.29208086995 +34.67892063113 14.9698 14.4573 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.752#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54241_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 54241_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 09:00:12.41 +33:44:54.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54243_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 54243_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 09:00:17.09 +34:29:56.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54245_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 54245_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 09:22:39.01 +27:45:31.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.54, MAG_FAINT_SEARCH_LIMIT=15.52)GAIADR2_OUTPUT=# 2.467 695272952305665792 140.66181022814 +27.75891947540 14.6166 13.9179 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.467#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54246_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 54246_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 09:04:58.54 +32:09:27.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.48, MAG_FAINT_SEARCH_LIMIT=15.46)
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Considering the candidate 54247_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 54247_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 09:33:25.26 +31:58:59.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)GAIADR2_OUTPUT=# 1.459 697950091320752768 143.35496666293 +31.98363192257 14.3522 13.6461 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.459#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54250_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 54250_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 08:56:55.69 +28:30:14.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.19, MAG_FAINT_SEARCH_LIMIT=15.17)
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Considering the candidate 54257_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 54257_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 09:01:52.79 +27:38:30.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54258_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 54258_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 09:20:02.64 +26:40:13.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54431_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 54431_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 08:44:22.67 +28:26:25.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54557_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 54557_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 09:22:14.11 +31:53:14.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54708_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 54708_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 09:36:44.34 +32:25:11.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54933_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 54933_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 09:00:11.87 +33:04:27.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55027_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 55027_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 08:54:29.54 +26:55:10.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55251_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 55251_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 09:13:25.20 +30:06:22.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55286_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 55286_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 08:43:01.84 +33:36:28.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55769_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 55769_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 08:56:50.44 +27:03:59.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55786_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
Preparing report for the candidate 55786_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
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Considering the candidate 55801_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 55801_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 08:40:40.63 +31:15:08.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55892_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 55892_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 09:25:50.23 +28:30:35.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55915_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 55915_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 09:36:55.68 +33:34:43.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55946_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 55946_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 09:16:11.41 +34:42:37.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55973_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 55973_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 09:34:28.40 +32:29:43.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.63, MAG_FAINT_SEARCH_LIMIT=15.61)GAIADR2_OUTPUT=# 2.986 698038567647024384 143.61855401520 +32.49469180592 14.8886 14.4345 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.986#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56026_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 56026_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 09:29:02.45 +32:09:22.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.73, MAG_FAINT_SEARCH_LIMIT=15.71)GAIADR2_OUTPUT=# 1.063 700932654049848576 142.26036374221 +32.15601349806 14.9224 14.2978 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.063#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56125_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 56125_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 09:19:59.54 +25:41:30.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56168_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 56168_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 08:44:17.53 +32:02:04.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56172_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 56172_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 09:23:59.70 +26:39:40.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56178_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
Preparing report for the candidate 56178_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
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Considering the candidate 56203_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 56203_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 09:36:15.61 +30:24:59.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.82, MAG_FAINT_SEARCH_LIMIT=15.80)GAIADR2_OUTPUT=# 1.200 696778011925330688 144.06466552082 +30.41647848312 14.8633 14.4557 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.200#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56211_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 56211_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 09:04:26.24 +34:29:46.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56212_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 56212_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 09:28:39.81 +34:14:31.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56219_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 56219_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 09:21:21.98 +27:10:36.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.96, MAG_FAINT_SEARCH_LIMIT=15.94)GAIADR2_OUTPUT=# 1.250 694863452943743104 140.34123147284 +27.17657196629 15.2446 14.7584 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.250#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56228_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 56228_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 08:57:46.05 +26:55:58.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56232_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 56232_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 09:17:29.26 +26:36:00.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56238_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 56238_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 08:27:05.38 +25:30:08.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.70, MAG_FAINT_SEARCH_LIMIT=15.68)GAIADR2_OUTPUT=# 0.900 679595565761318784 126.77218254864 +25.50233875119 14.8395 14.2565 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.900#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56258_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 56258_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 08:49:45.24 +26:23:03.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56275_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 56275_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 09:36:14.20 +32:37:52.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56278_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 56278_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 09:28:55.94 +31:35:46.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.88, MAG_FAINT_SEARCH_LIMIT=15.86)GAIADR2_OUTPUT=# 1.596 700881629838436352 142.23360299017 +31.59619814098 15.1062 14.5934 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.596#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56280_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 56280_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 09:19:19.08 +33:52:50.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56282_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 56282_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 09:06:31.53 +27:35:19.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56286_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 56286_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 08:26:48.39 +26:08:24.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.88, MAG_FAINT_SEARCH_LIMIT=15.86)GAIADR2_OUTPUT=# 1.744 679906074716369280 126.70202575276 +26.13978649016 14.8079 14.0011 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.744#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56294_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 56294_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 08:38:03.10 +33:45:42.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.92, MAG_FAINT_SEARCH_LIMIT=15.90)GAIADR2_OUTPUT=# 1.493 711121278548326656 129.51341523663 +33.76168035222 14.6057 13.5394 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.493#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56313_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 56313_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 09:33:06.26 +27:31:57.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56314_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 56314_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 09:29:15.94 +32:34:16.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.90, MAG_FAINT_SEARCH_LIMIT=15.88)GAIADR2_OUTPUT=# 0.362 701088338024412032 142.31641994539 +32.57103837984 15.0427 14.5505 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.362#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56322_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 56322_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 09:26:17.73 +30:35:21.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56337_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 56337_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 09:20:34.11 +31:50:43.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.74, MAG_FAINT_SEARCH_LIMIT=15.72)GAIADR2_OUTPUT=# 0.875 700713129681109248 140.14184016711 +31.84552166326 14.4845 13.6889 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.875#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56358_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 56358_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 09:17:56.54 +33:58:21.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56385_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 56385_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks
**** FOUND 09:04:34.93 +33:35:02.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 12972_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126
The candidate 12972_fd_Cnc-01-Q1b1x1_2026-04-17_00-35-12_20.00sec_-5.00C_LIGHTs_0126 did not pass the final checks