This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS
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,2461144.6857,14.09,0.05,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 20260414.1857 14.09CV 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,2461144.6857,14.82,0.05,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 20260414.1857 14.82CV 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,2461144.6857,14.76,0.05,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 20260414.1857 14.76CV 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,2461144.6857,14.73,0.05,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 20260414.1857 14.73CV 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: 2461144.68609503 14.04.2026 04:27:48.611 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 9
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: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 9188
Objects passed selection criteria: 9177
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: 8501.75
Average stars matched: 8074.75 (94.9775 %)
Memory usage VmPeak: 114164 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 13 23:29:47 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: 2461144.68609503 14.04.2026 04:27:48.611 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 55
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: 16 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): 51354
Objects passed selection criteria: 51228
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: 48004.5
Average stars matched: 45809.8 (95.428 %)
Memory usage VmPeak: 148300 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 13 23:30:39 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_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.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_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.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: 2461144.68531331
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
'tns_transients_list.txt' -> '../tns_transients_list.txt'
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_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits exists and is non-empty
Saving wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits to local_wcs_cache/
'wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits' -> 'local_wcs_cache/wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits'
wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits exists and is non-empty
Saving wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits to local_wcs_cache/
'wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits' -> 'local_wcs_cache/wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:59:59.815 +30:00:01.62
Second-epoch image center 08:59:53.708 +29:54:56.74
Angular distance between the image centers 0.0875 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:59:59.815 +30:00:01.62
Second-epoch image center 08:59:56.793 +29:55:21.92
Angular distance between the image centers 0.0785 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 08:59:53.708 +29:54:56.74
Second-epoch second image center 08:59:56.793 +29:55:21.92
Angular distance between the image centers 0.01316 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.tHXaz9B5eB
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.haQ3XfMtnK
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_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits &> /tmp/tmp.4UNDyExQCU
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits &> /tmp/tmp.JWPHwkwwRD
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.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 9 candidate transients before the final filtering. (Hard limit: 3000)
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
2.2 pix fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits
2.2 pix fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.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
15.3 mag. fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits
15.3 mag. fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits
All-image limiting magnitude estimate: 15.3 (SNR ) 12.2 (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.tHXaz9B5eB (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_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/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.haQ3XfMtnK (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_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/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.4UNDyExQCU (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_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.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_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits
WCS-calibrated image found: wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits
Checking if the catalog wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits.cat corresponding to the image wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits.cat corresponding to the image wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.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_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits
WCS catalog name: wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.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=8892
Got 8892 stars (including 8356 good ones) from the SExtractor catalog wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits.cat
util/solve_plate_with_UCAC5 got 8892 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (37.6 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 628 (Dec 23.9 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(), 948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 8799 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 569 to 628 (Dec 23.9 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(), 8797 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 8797 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits -region wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.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.JWPHwkwwRD (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_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.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_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits
WCS-calibrated image found: wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits
Checking if the catalog wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits.cat corresponding to the image wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits.cat corresponding to the image wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.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_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits
WCS catalog name: wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=538, passed=8764
Got 8764 stars (including 8221 good ones) from the SExtractor catalog wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits.cat
util/solve_plate_with_UCAC5 got 8764 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (37.6 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 628 (Dec 24.0 to 35.4)
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(), 948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 8676 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 569 to 628 (Dec 24.0 to 35.4)
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(), 8678 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 8678 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
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_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits -region wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.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_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/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_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/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_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits'
Saving fully-calibrated image wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits'
Preparing the HTML report for the field Cnc-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20795.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20802.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20738_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 20738_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 09:00:51.56 +30:06:25.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20758_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 20758_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 09:26:27.12 +28:39:42.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20772_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 20772_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 08:43:32.14 +26:36:57.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20790_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 20790_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 08:52:44.12 +30:23:02.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20795_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 20795_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 09:03:01.45 +28:37:06.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 0.194 693190438630390144 135.75610111742 +28.61840182301 12.1064 11.6787 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.194#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20796_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 20796_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 08:59:23.24 +28:47:52.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20797_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 20797_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 08:26:59.90 +29:33:53.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20799_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 20799_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 08:49:54.63 +28:59:11.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20802_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 20802_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 08:54:10.72 +29:56:56.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 0.628 705516445009779328 133.54485215672 +29.94917884588 12.1314 11.6218 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.628#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
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_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.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_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.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_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.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_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits exists and is non-empty
wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:59:59.815 +30:00:01.62
Second-epoch image center 08:59:53.708 +29:54:56.74
Angular distance between the image centers 0.0875 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:59:59.815 +30:00:01.62
Second-epoch image center 08:59:56.793 +29:55:21.92
Angular distance between the image centers 0.0785 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 08:59:53.708 +29:54:56.74
Second-epoch second image center 08:59:56.793 +29:55:21.92
Angular distance between the image centers 0.01316 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.Vtn4fdmngQ
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.aMA9hrnRRL
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_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits &> /tmp/tmp.4epdHpR2SM
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits &> /tmp/tmp.sOBpt6I26i
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.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 47 candidate transients before the final filtering. (Hard limit: 3000)
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
2.2 pix fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits
2.1 pix fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.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
15.4 mag. fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits
15.4 mag. fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits
All-image limiting magnitude estimate: 15.4 (SNR ) 14.7 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.Vtn4fdmngQ (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_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/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.aMA9hrnRRL (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_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/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.4epdHpR2SM (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_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.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_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits
WCS-calibrated image found: wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits
Checking if the catalog wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits.cat corresponding to the image wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits.cat corresponding to the image wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.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_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits
WCS catalog name: wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=2082, passed=46522
Got 46522 stars (including 44365 good ones) from the SExtractor catalog wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits.cat
util/solve_plate_with_UCAC5 got 46522 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (37.6 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 628 (Dec 23.9 to 35.4)
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(), 945 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 46105 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 569 to 628 (Dec 23.9 to 35.4)
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(), 46106 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 46106 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
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_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits -region wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.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.sOBpt6I26i (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_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.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_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits
WCS-calibrated image found: wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits
Checking if the catalog wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits.cat corresponding to the image wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits.cat corresponding to the image wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.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_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits
WCS catalog name: wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=2176, passed=47838
Got 47838 stars (including 45601 good ones) from the SExtractor catalog wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits.cat
util/solve_plate_with_UCAC5 got 47838 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (37.6 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 23.9 to 35.4)
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(), 944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 47420 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 569 to 629 (Dec 23.9 to 35.4)
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(), 47421 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 47421 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
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_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits -region wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.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_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/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_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/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_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.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_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-26-41_20.00sec_-4.90C_LIGHTs_0119.fits
Saving fully-calibrated image wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.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_2026-04-13_CI_Cnc-01-Q1b1x1_232846_TTUQ1b1x1_25313_MeH33ShS/wcs_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120.fits
Preparing the HTML report for the field Cnc-01-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out54237.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56103.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56109.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56152.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56224.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56241.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56246.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56290.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56306.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56315.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56321.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56326.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56331.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56342.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56354.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56360.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56376.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out56071.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out55539.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56199.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56317.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56328.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54237_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 54237_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 09:12:19.48 +31:18:19.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.73, MAG_FAINT_SEARCH_LIMIT=15.71)GAIADR2_OUTPUT=# 1.586 699965942810463232 138.08067492478 +31.30514518464 14.9531 14.4351 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.586#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54409_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 54409_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 08:44:22.53 +28:26:24.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54527_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 54527_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 09:22:14.05 +31:53:14.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54690_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 54690_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 09:36:44.34 +32:25:11.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54994_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 54994_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 08:54:29.54 +26:55:10.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55127_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 55127_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 08:42:22.88 +29:15:23.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55246_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 55246_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 08:43:01.85 +33:36:28.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55539_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
Preparing report for the candidate 55539_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
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Considering the candidate 55558_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 55558_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 08:40:40.64 +31:15:07.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55804_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 55804_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 09:36:55.66 +33:34:42.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55981_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 55981_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 09:19:10.42 +26:57:34.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56040_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 56040_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 09:28:36.16 +29:57:55.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56068_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 56068_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 08:26:49.89 +34:39:26.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56071_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 56071_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 09:30:17.40 +26:38:28.4 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)
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Considering the candidate 56103_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 56103_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 09:04:34.92 +33:35:02.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.60, MAG_FAINT_SEARCH_LIMIT=15.58)GAIADR2_OUTPUT=# 2.007 712639635386917376 136.14516339921 +33.58360163828 14.8155 14.2683 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.007#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56109_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 56109_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 09:32:06.76 +27:02:27.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.77, MAG_FAINT_SEARCH_LIMIT=15.75)GAIADR2_OUTPUT=# 1.152 694294696193266432 143.02805141769 +27.04121972608 14.9719 14.3678 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.152#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56113_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 56113_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 09:06:31.40 +27:35:20.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56152_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 56152_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 08:28:29.00 +33:25:55.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.79, MAG_FAINT_SEARCH_LIMIT=15.77)GAIADR2_OUTPUT=# 0.840 903016637762048768 127.12074571921 +33.43219380210 14.9609 14.4409 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.840#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56196_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 56196_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 09:20:58.37 +27:29:38.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56199_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
Preparing report for the candidate 56199_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
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Considering the candidate 56212_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 56212_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 09:25:39.62 +32:17:47.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56224_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 56224_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 09:20:04.21 +33:29:02.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.85, MAG_FAINT_SEARCH_LIMIT=15.83)GAIADR2_OUTPUT=# 1.082 702091401866362880 140.01753720292 +33.48381045572 14.8195 14.2452 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.082#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56233_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 56233_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 08:33:02.95 +25:30:57.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56241_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 56241_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 09:21:58.51 +34:15:56.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.88, MAG_FAINT_SEARCH_LIMIT=15.86)GAIADR2_OUTPUT=# 1.145 702327865586657152 140.49342666005 +34.26548250044 14.9598 14.3672 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.145#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56244_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 56244_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 09:26:17.77 +30:35:21.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56246_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 56246_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 08:47:33.48 +28:40:37.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.78, MAG_FAINT_SEARCH_LIMIT=15.76)
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Considering the candidate 56249_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 56249_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 09:28:38.38 +31:52:06.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56290_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 56290_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 09:24:14.43 +29:39:02.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.85, MAG_FAINT_SEARCH_LIMIT=15.83)GAIADR2_OUTPUT=# 0.315 697236027237829888 141.06015668077 +29.65086081134 15.0716 14.4962 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.315#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56291_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 56291_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 09:35:03.02 +32:45:36.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56306_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 56306_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 08:51:22.80 +29:06:32.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.91, MAG_FAINT_SEARCH_LIMIT=15.89)GAIADR2_OUTPUT=# 1.126 705090972667051776 132.84532685265 +29.10892794919 14.8811 14.3792 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.126#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56313_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 56313_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 08:29:16.97 +31:56:09.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56315_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 56315_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 09:32:15.13 +34:05:00.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.86, MAG_FAINT_SEARCH_LIMIT=15.84)GAIADR2_OUTPUT=# 0.876 797460669637841536 143.06331283217 +34.08332317683 14.8652 14.2949 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.876#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56317_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
Preparing report for the candidate 56317_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
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Considering the candidate 56321_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 56321_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 08:52:26.39 +31:09:20.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.89, MAG_FAINT_SEARCH_LIMIT=15.87)GAIADR2_OUTPUT=# 0.575 706659391643390080 133.11005933407 +31.15564330078 14.9154 14.4493 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.575#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56326_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 56326_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 09:24:26.03 +30:49:15.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.89, MAG_FAINT_SEARCH_LIMIT=15.87)GAIADR2_OUTPUT=# 0.900 700361938795335296 141.10820394937 +30.82114953104 15.0558 14.6905 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 56328_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
Preparing report for the candidate 56328_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
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Considering the candidate 56331_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 56331_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 09:28:18.21 +31:35:25.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.86, MAG_FAINT_SEARCH_LIMIT=15.84)GAIADR2_OUTPUT=# 0.884 700876510237410944 142.07571535802 +31.59053793377 14.9928 14.5287 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.884#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56342_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 56342_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 09:22:25.53 +33:06:34.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.96, MAG_FAINT_SEARCH_LIMIT=15.94)GAIADR2_OUTPUT=# 0.344 702007147491286400 140.60626996190 +33.10959255948 14.9782 14.3373 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.344#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56343_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 56343_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 09:19:18.90 +33:52:49.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56351_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 56351_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 09:36:03.53 +31:28:17.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56354_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 56354_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 09:26:33.24 +28:38:36.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.82, MAG_FAINT_SEARCH_LIMIT=15.80)GAIADR2_OUTPUT=# 1.053 695439871914781184 141.63835172232 +28.64373423935 14.7904 14.2373 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.053#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56360_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 56360_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 08:29:18.01 +25:24:31.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.88, MAG_FAINT_SEARCH_LIMIT=15.86)GAIADR2_OUTPUT=# 0.641 679623878186274688 127.32504617419 +25.40901135791 14.8213 14.1777 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.641#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56362_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 56362_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 09:33:06.21 +27:31:56.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56364_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 56364_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 09:08:20.95 +34:36:14.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56369_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 56369_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 09:25:50.32 +28:30:35.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56376_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 56376_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks
**** FOUND 08:49:45.18 +26:23:02.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.88, MAG_FAINT_SEARCH_LIMIT=15.86)GAIADR2_OUTPUT=# 1.269 691201460748462464 132.43852824913 +26.38433259501 15.0807 14.6078 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.269#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 12972_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120
The candidate 12972_fd_Cnc-01-Q1b1x1_2026-04-13_23-27-48_20.00sec_-5.00C_LIGHTs_0120 did not pass the final checks