This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR
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,2461149.7109,14.28,0.05,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 20260419.2109 14.28CV 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,2461149.7109,14.81,0.05,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 20260419.2109 14.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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,2461149.7109,14.86,0.05,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 20260419.2109 14.86CV 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
AT Cnc,2461149.7109,13.23,0.05,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
AT Cnc 20260419.2109 13.23CV 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
CSS_J085921.0+273501,2461149.7109,13.72,0.05,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
CSS_J085921.0+273501 20260419.2109 13.72CV 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: 2461149.71120839 19.04.2026 05:03:58.405 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.56
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 8926
Objects passed selection criteria: 8919
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: 8285.75
Average stars matched: 7935.25 (95.7698 %)
Memory usage VmPeak: 113968 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Apr 19 00:10:05 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: 2461149.71120839 19.04.2026 05:03:58.405 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 74
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.27
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: 18 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): 52185
Objects passed selection criteria: 52039
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: 48856.5
Average stars matched: 46323 (94.8144 %)
Memory usage VmPeak: 149368 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Apr 19 00:11:03 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_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.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_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.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: 2461149.71051385
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
'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_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits exists and is non-empty
Saving wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits to local_wcs_cache/
'wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits' -> 'local_wcs_cache/wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits'
wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits exists and is non-empty
Saving wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits to local_wcs_cache/
'wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits' -> 'local_wcs_cache/wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits (1st reference image)
verification OK: wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits
Image size: 941.6'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 08:59:59.815 +30:00:01.62 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits (1st new image)
verification OK: wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits
Image size: 941.4'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:00:07.625 +29:58:20.01 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:59:59.815 +30:00:01.62
Second-epoch image center 09:00:07.625 +29:58:20.01
Angular distance between the image centers 0.0399 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits (2nd new image)
verification OK: wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits
Image size: 941.4'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:00:05.022 +29:58:10.61 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:59:59.815 +30:00:01.62
Second-epoch image center 09:00:05.022 +29:58:10.61
Angular distance between the image centers 0.0361 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 09:00:07.625 +29:58:20.01
Second-epoch second image center 09:00:05.022 +29:58:10.61
Angular distance between the image centers 0.00975 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.9wthva6Mkl
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.ttj7HvX7fR
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_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits &> /tmp/tmp.d8lPkuA5v7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits &> /tmp/tmp.BnxNd45NXb
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.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 2 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits
2.0 pix Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits
2.1 pix fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits
2.1 pix fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.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_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits
15.3 mag. fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.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.9wthva6Mkl (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_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/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.ttj7HvX7fR (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_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/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.d8lPkuA5v7 (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_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.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_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits
WCS-calibrated image found: wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits
Checking if the catalog wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits.cat corresponding to the image wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits.cat corresponding to the image wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.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_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits
WCS catalog name: wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=582, passed=8473
Got 8473 stars (including 7879 good ones) from the SExtractor catalog wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits.cat
util/solve_plate_with_UCAC5 got 8473 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 629 (Dec 24.0 to 35.5)
Done reading UCAC5 zone files...
Matched 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(), 947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 8392 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 570 to 629 (Dec 24.0 to 35.5)
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(), 8392 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 8392 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits -region wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.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.BnxNd45NXb (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_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.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_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits
WCS-calibrated image found: wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits
Checking if the catalog wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits.cat corresponding to the image wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits.cat corresponding to the image wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.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_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits
WCS catalog name: wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=584, passed=8326
Got 8326 stars (including 7736 good ones) from the SExtractor catalog wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits.cat
util/solve_plate_with_UCAC5 got 8326 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 629 (Dec 24.0 to 35.5)
Done reading UCAC5 zone files...
Matched 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(), 947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 8254 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 570 to 629 (Dec 24.0 to 35.5)
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(), 8255 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 8255 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits -region wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.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_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/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_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/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_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits'
Saving fully-calibrated image wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits'
Preparing the HTML report for the field Cnc-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20783.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: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20772_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 20772_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 09:26:27.13 +28:39:43.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20783_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 20783_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 08:43:32.14 +26:36:57.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 0.301 703182564077764736 130.88399533601 +26.61596178565 11.9588 11.4388 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.301#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: 2s
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_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.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_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.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_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.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_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits exists and is non-empty
wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits (1st reference image)
verification OK: wcs_Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits
Image size: 941.6'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 08:59:59.815 +30:00:01.62 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits (1st new image)
verification OK: wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Image size: 941.4'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:00:07.625 +29:58:20.01 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:59:59.815 +30:00:01.62
Second-epoch image center 09:00:07.625 +29:58:20.01
Angular distance between the image centers 0.0399 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits (2nd new image)
verification OK: wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits
Image size: 941.4'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:00:05.022 +29:58:10.61 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:59:59.815 +30:00:01.62
Second-epoch image center 09:00:05.022 +29:58:10.61
Angular distance between the image centers 0.0361 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 09:00:07.625 +29:58:20.01
Second-epoch second image center 09:00:05.022 +29:58:10.61
Angular distance between the image centers 0.00975 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.M0sVKVPBy5
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.yIpyTJ3N5a
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_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits &> /tmp/tmp.nCrIy3NwZH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits &> /tmp/tmp.YFVVZVNrW7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.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 63 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
1.9 pix Cnc-01-Q1b1x1_2026-02-11_00-23-48_20.00sec_-14.90C_LIGHT_0249.fits
1.8 pix Cnc-01-Q1b1x1_2026-02-11_00-24-30_20.00sec_-15.00C_LIGHT_0250.fits
2.0 pix fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits
2.0 pix fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.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_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits
15.4 mag. fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.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.M0sVKVPBy5 (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_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/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.yIpyTJ3N5a (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_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/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.nCrIy3NwZH (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_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.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_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits
WCS-calibrated image found: wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits
Checking if the catalog wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits.cat corresponding to the image wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits.cat corresponding to the image wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.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_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits
WCS catalog name: wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=2308, passed=48636
Got 48636 stars (including 46246 good ones) from the SExtractor catalog wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits.cat
util/solve_plate_with_UCAC5 got 48636 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 569 to 629 (Dec 24.0 to 35.5)
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 943 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 48170 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 569 to 629 (Dec 24.0 to 35.5)
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 48171 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 48171 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
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_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits -region wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.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.YFVVZVNrW7 (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_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.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_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits
WCS-calibrated image found: wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits
Checking if the catalog wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits.cat corresponding to the image wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits.cat corresponding to the image wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.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_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits
WCS catalog name: wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=2295, passed=49275
Got 49275 stars (including 46897 good ones) from the SExtractor catalog wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits.cat
util/solve_plate_with_UCAC5 got 49275 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 569 to 629 (Dec 24.0 to 35.5)
Done reading UCAC5 zone files...
Matched 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(), 941 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 48873 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 569 to 629 (Dec 24.0 to 35.5)
Done reading UCAC5 zone files...
Matched 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(), 48874 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 48874 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
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_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits -region wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.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_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/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_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/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_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.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_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-02-58_20.00sec_-4.90C_LIGHTs_0365.fits
Saving fully-calibrated image wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.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_2026-04-19_CI_Cnc-01-Q1b1x1_000451_TTUQ1b1x1_3555548_3qELeSAR/wcs_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366.fits
Preparing the HTML report for the field Cnc-01-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out54255.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54257.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54442.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54681.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54709.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55348.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56218.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56258.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56380.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56392.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56401.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56431.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56523.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56530.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56531.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56547.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56569.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56580.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56591.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out12972.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55905.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56349.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56669.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 4s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54251_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 54251_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 09:00:12.40 +33:44:54.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54252_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 54252_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 09:07:38.25 +34:55:58.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54255_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 54255_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 09:07:38.34 +29:24:28.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.76, MAG_FAINT_SEARCH_LIMIT=15.74)GAIADR2_OUTPUT=# 0.984 699235764010233600 136.90954578332 +29.40765355453 14.6012 14.0513 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.984#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54256_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 54256_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 09:09:41.08 +32:27:12.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54257_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 54257_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 09:22:40.14 +27:45:26.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.76, MAG_FAINT_SEARCH_LIMIT=15.74)GAIADR2_OUTPUT=# 3.164 695272883586188928 140.66810729768 +27.75691753034 14.7306 14.2412 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.164#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54260_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 54260_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 09:29:20.51 +30:06:33.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54261_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 54261_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 08:55:13.71 +26:23:48.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54262_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 54262_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 09:02:40.66 +31:26:42.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54265_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 54265_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 08:55:32.75 +33:49:41.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54266_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 54266_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 09:01:52.79 +27:38:30.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54442_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 54442_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 08:44:22.51 +28:26:24.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.40, MAG_FAINT_SEARCH_LIMIT=12.38)GAIADR2_OUTPUT=# 0.051 705170171864290432 131.09379852324 +28.44023732742 11.1101 10.4142 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.051#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54558_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 54558_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 09:22:14.08 +31:53:14.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54663_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 54663_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 09:17:33.25 +26:26:42.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54681_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 54681_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 09:04:15.08 +34:32:42.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 0.536 713468357916656256 136.06265682678 +34.54514304321 12.6772 12.2046 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.536#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54709_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 54709_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 09:36:44.37 +32:25:11.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 0.790 794055207249079040 144.18513248663 +32.41989136236 12.4254 11.6117 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.790#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54976_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 54976_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 09:00:11.86 +33:04:27.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55064_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 55064_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 09:17:35.68 +29:19:36.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55222_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 55222_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 09:13:25.24 +30:06:22.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55348_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 55348_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 08:43:01.85 +33:36:28.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 0.292 710409001172505216 130.75761207788 +33.60782089330 13.6582 12.9554 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.292#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 55634_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 55634_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 09:02:10.00 +33:19:15.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55831_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 55831_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 08:40:40.54 +31:15:08.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55873_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 55873_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 09:36:55.67 +33:34:42.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55905_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
Preparing report for the candidate 55905_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
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Considering the candidate 55967_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 55967_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 09:30:17.21 +26:38:27.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55991_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 55991_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 09:19:41.44 +33:44:17.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56144_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 56144_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 09:24:46.69 +24:58:21.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56165_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 56165_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 09:20:22.03 +28:12:35.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56218_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 56218_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 09:26:34.56 +26:10:50.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.81, MAG_FAINT_SEARCH_LIMIT=15.79)GAIADR2_OUTPUT=# 0.798 693764387991550336 141.64423137882 +26.18047835497 14.8988 14.3307 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.798#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56258_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 56258_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 09:24:19.08 +28:51:59.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.80, MAG_FAINT_SEARCH_LIMIT=15.78)GAIADR2_OUTPUT=# 2.673 695484986251183232 141.07959839035 +28.86720963834 14.7740 13.8776 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.673#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56299_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 56299_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 09:37:00.80 +34:01:48.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56342_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 56342_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 09:26:17.65 +30:35:21.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56349_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
Preparing report for the candidate 56349_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
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Considering the candidate 56380_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 56380_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 09:22:08.60 +32:37:58.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.81, MAG_FAINT_SEARCH_LIMIT=15.79)GAIADR2_OUTPUT=# 2.430 700869947527305344 140.53507280846 +32.63259205763 14.8896 14.3350 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.430#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56383_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 56383_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 09:20:49.98 +33:51:00.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56392_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 56392_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 08:54:35.96 +25:39:53.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.76, MAG_FAINT_SEARCH_LIMIT=15.74)GAIADR2_OUTPUT=# 0.198 690156684183083776 133.64985481895 +25.66472628965 14.9267 14.3726 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.198#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56396_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 56396_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 09:20:04.24 +33:29:02.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56401_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 56401_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 09:32:12.75 +31:18:44.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.88, MAG_FAINT_SEARCH_LIMIT=15.86)GAIADR2_OUTPUT=# 0.859 697819799192658176 143.05310993198 +31.31206731506 15.0240 14.5330 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.859#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56403_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 56403_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 09:28:40.00 +34:14:31.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56408_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 56408_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 09:28:03.02 +34:19:32.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56427_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 56427_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 08:59:51.74 +34:07:46.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56429_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 56429_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 08:26:50.04 +34:39:24.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56431_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 56431_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 09:31:53.30 +33:37:44.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.80, MAG_FAINT_SEARCH_LIMIT=15.78)GAIADR2_OUTPUT=# 0.799 797238568289179776 142.97229552502 +33.62889345678 14.8020 14.0515 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.799#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56435_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 56435_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 09:25:39.64 +32:17:47.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56471_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 56471_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 09:33:06.26 +27:31:56.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56472_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 56472_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 09:34:28.47 +32:29:43.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56484_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 56484_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 08:33:02.97 +25:30:58.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56488_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 56488_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 09:27:07.53 +34:15:54.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56490_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 56490_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 09:26:23.70 +28:54:36.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56502_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 56502_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 09:36:03.46 +31:28:17.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56504_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 56504_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 09:25:50.36 +28:30:35.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56523_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 56523_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 09:32:15.88 +30:37:09.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.93, MAG_FAINT_SEARCH_LIMIT=15.91)GAIADR2_OUTPUT=# 0.737 697573302430194304 143.06639471785 +30.61919198827 15.0457 14.4081 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.737#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56524_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 56524_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 08:57:46.07 +26:55:58.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56530_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 56530_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 09:03:28.05 +31:06:00.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.96, MAG_FAINT_SEARCH_LIMIT=15.94)GAIADR2_OUTPUT=# 2.449 711725357109201664 135.86612784424 +31.09982441143 15.2100 14.4970 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.449#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56531_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 56531_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 09:32:52.14 +25:37:11.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.84, MAG_FAINT_SEARCH_LIMIT=15.82)GAIADR2_OUTPUT=# 0.158 645832101995894528 143.21720436787 +25.61981843108 14.7574 14.2793 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.158#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56534_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 56534_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 08:49:45.22 +26:23:04.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56547_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 56547_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 08:31:23.02 +34:22:53.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.96, MAG_FAINT_SEARCH_LIMIT=15.94)GAIADR2_OUTPUT=# 0.579 903540211455370880 127.84605048679 +34.38127180924 15.0012 14.4383 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.579#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56569_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 56569_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 09:16:16.41 +30:33:00.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.88, MAG_FAINT_SEARCH_LIMIT=15.86)GAIADR2_OUTPUT=# 1.068 699122406937663488 139.06810591809 +30.54989813468 15.6637 15.3141 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.068#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56580_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 56580_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 08:29:12.85 +30:24:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.81, MAG_FAINT_SEARCH_LIMIT=15.79)GAIADR2_OUTPUT=# 1.089 708042130594026624 127.30321291665 +30.41300546998 14.8546 14.2271 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.089#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56588_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 56588_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks
**** FOUND 09:17:29.22 +26:35:59.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56591_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366
The candidate 56591_fd_Cnc-01-Q1b1x1_2026-04-19_00-03-58_20.00sec_-4.90C_LIGHTs_0366 did not pass the final checks