This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI
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!
TCP 2026 04 16.1979* 09 36 26.20 +26 01 57.9 14.0 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461146.6979,14.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260416.1979 14.03CV 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!
TCP 2026 04 16.1979* 09 43 07.94 +21 10 59.0 14.2 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J145.7855+21.1825,2461146.6979,14.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J145.7855+21.1825 20260416.1979 14.22CV 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,2461146.6979,14.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260416.1979 14.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 16.1979* 09 29 38.43 +24 09 54.6 14.4 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461146.6979,14.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260416.1979 14.37CV 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,2461146.6979,14.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260416.1979 14.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461119.67641736 20.03.2026 04:13:52.460 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
First image: 2461119.67641736 20.03.2026 04:13:52.460 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
Last image: 2461146.69817459 16.04.2026 04:45:12.285 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 7
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.60
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 6917
Objects passed selection criteria: 6915
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 6634
Average stars matched: 6484.5 (97.7465 %)
Memory usage VmPeak: 113188 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 15 18:49:36 CDT 2026
VaST build number 1.0rc89-18-ga9a0ae89
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Apr 15 23:49:22 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461119.67641736 20.03.2026 04:13:52.460 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
First image: 2461119.67641736 20.03.2026 04:13:52.460 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
Last image: 2461146.69817459 16.04.2026 04:45:12.285 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 199
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.32
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 19 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): 35340
Objects passed selection criteria: 35264
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: 32952
Average stars matched: 31640 (96.0185 %)
Memory usage VmPeak: 139292 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 15 18:49:36 CDT 2026
VaST build number 1.0rc89-18-ga9a0ae89
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-15)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Apr 15 23:50:25 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits
SExtractor catalog cache: saved Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat to cache
SExtractor catalog cache: saved Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.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: 2461146.69763654
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits exists and is non-empty
Saving wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits to local_wcs_cache/
'wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits' -> 'local_wcs_cache/wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits'
wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits exists and is non-empty
Saving wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits to local_wcs_cache/
'wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits' -> 'local_wcs_cache/wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits'
wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits exists and is non-empty
Saving wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits to local_wcs_cache/
'wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits' -> 'local_wcs_cache/wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits'
wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits exists and is non-empty
Saving wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits to local_wcs_cache/
'wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits' -> 'local_wcs_cache/wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits (1st reference image)
verification OK: wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 09:14:05.815 +22:02:06.51 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits (1st new image)
verification OK: wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits
Image size: 936.8'x623.9' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 09:14:00.451 +21:58:42.66 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:14:05.815 +22:02:06.51
Second-epoch image center 09:14:00.451 +21:58:42.66
Angular distance between the image centers 0.0603 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits (2nd new image)
verification OK: wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits
Image size: 936.8'x623.9' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 09:13:59.844 +21:58:57.62 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:14:05.815 +22:02:06.51
Second-epoch image center 09:13:59.844 +21:58:57.62
Angular distance between the image centers 0.0573 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 09:14:00.451 +21:58:42.66
Second-epoch second image center 09:13:59.844 +21:58:57.62
Angular distance between the image centers 0.00477 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits &> /tmp/tmp.VT3ksyK2DZ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits &> /tmp/tmp.GDmbqf7oXt
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits &> /tmp/tmp.tMSTWCEMgC
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits &> /tmp/tmp.mFradKxRUZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits and wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits and wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat
Found non-empty wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits and wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat
The reference image (wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits) and catalog (wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat) found
'wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat' -> 'wcsmag.cat'
Read 9535 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 129.8640 to 147.3424 deg, Dec +16.4979 to +27.3084 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 129.8640 to 147.3424 deg, Dec 16.4979 to 27.3084 deg
Loaded 5782 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): 4541 out of 4760 total matches.
Matched with Tycho-2 4760 out of 9535 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.916671
a=0.000000 b=1.000000 c=22.916671
From vast_summary.log: estimated ref. image limiting mag.: -7.60
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.32
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.32
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.5 pix Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
2.3 pix Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
2.9 pix fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits
2.9 pix fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits
Limiting magnitude estimates:
15.3 mag. Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
15.4 mag. Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
15.1 mag. fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits
15.1 mag. fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 12.4 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.VT3ksyK2DZ (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_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits' -> 'wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
WCS_IMAGE_NAME=wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
WCS-calibrated image found: wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
Checking if the catalog wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat corresponding to the image wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits alredy exist and is non-empty...
Catalog wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat corresponding to the image wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
WCS catalog name: wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=608, passed=9535
Got 9535 stars (including 8921 good ones) from the SExtractor catalog wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat
util/solve_plate_with_UCAC5 got 9535 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 945 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 9415 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 9417 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 9417 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits -region wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.GDmbqf7oXt (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_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits' -> 'wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
WCS_IMAGE_NAME=wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
WCS-calibrated image found: wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
Checking if the catalog wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits.cat corresponding to the image wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits alredy exist and is non-empty...
Catalog wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits.cat corresponding to the image wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
WCS catalog name: wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=669, passed=9214
Got 9214 stars (including 8536 good ones) from the SExtractor catalog wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits.cat
util/solve_plate_with_UCAC5 got 9214 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 9111 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 9110 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 9110 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits -region wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.tMSTWCEMgC (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_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.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_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits
WCS-calibrated image found: wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits
Checking if the catalog wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits.cat corresponding to the image wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits.cat corresponding to the image wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits
WCS catalog name: wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=859, passed=8680
Got 8680 stars (including 7817 good ones) from the SExtractor catalog wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits.cat
util/solve_plate_with_UCAC5 got 8680 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.8'
Seting catalog search parameters based on the expected field of view 936.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013011 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010409 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 8543 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 8543 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 8543 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Excluding outliers - 949 stars left (next iteration limit 1043)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits -region wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.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.mFradKxRUZ (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_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.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_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits
WCS-calibrated image found: wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits
Checking if the catalog wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits.cat corresponding to the image wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits.cat corresponding to the image wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits
WCS catalog name: wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=777, passed=8724
Got 8724 stars (including 7941 good ones) from the SExtractor catalog wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits.cat
util/solve_plate_with_UCAC5 got 8724 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.8'
Seting catalog search parameters based on the expected field of view 936.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013011 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010409 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 941 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 8623 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 8623 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 8623 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Excluding outliers - 949 stars left (next iteration limit 1043)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits -region wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits'
Saving fully-calibrated image wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits'
Saving fully-calibrated image wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits'
Saving fully-calibrated image wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits'
Preparing the HTML report for the field Cnc-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20208.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20313.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20319.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 20208_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 20208_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 09:10:26.42 +17:54:01.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.42, MAG_FAINT_SEARCH_LIMIT=13.40)GAIADR2_OUTPUT=# 0.605 635135881082287232 137.61019856924 +17.90059957269 12.2830 11.9053 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.605#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20209_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 20209_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 09:18:15.43 +18:23:09.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20313_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 20313_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 09:21:52.50 +22:38:34.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 0.409 639029251756023040 140.46886680470 +22.64284182102 12.2364 11.5925 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.409#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20319_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 20319_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 09:22:27.86 +23:50:42.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.50, MAG_FAINT_SEARCH_LIMIT=13.48)GAIADR2_OUTPUT=# 0.114 639403708480273280 140.61610570735 +23.84500371782 12.4183 11.7765 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.114#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-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits
SExtractor catalog cache: saved Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat to cache
SExtractor catalog cache: saved Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
Creating symlink local_wcs_cache/wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits exists and is non-empty
wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits exists and is non-empty
wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits exists and is non-empty
wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits (1st reference image)
verification OK: wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 09:14:05.815 +22:02:06.51 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits (1st new image)
verification OK: wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits
Image size: 936.8'x623.9' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 09:14:00.451 +21:58:42.66 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:14:05.815 +22:02:06.51
Second-epoch image center 09:14:00.451 +21:58:42.66
Angular distance between the image centers 0.0603 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits (2nd new image)
verification OK: wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits
Image size: 936.8'x623.9' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 09:13:59.844 +21:58:57.62 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:14:05.815 +22:02:06.51
Second-epoch image center 09:13:59.844 +21:58:57.62
Angular distance between the image centers 0.0573 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 09:14:00.451 +21:58:42.66
Second-epoch second image center 09:13:59.844 +21:58:57.62
Angular distance between the image centers 0.00477 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits &> /tmp/tmp.MZQqGy1Ha2
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits &> /tmp/tmp.pbK6B3P0sL
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits &> /tmp/tmp.80P1rRYEnz
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits &> /tmp/tmp.ByvP3dIiRN
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits and wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits and wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat
Found non-empty wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits and wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat
The reference image (wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits) and catalog (wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat) found
'wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat' -> 'wcsmag.cat'
Read 46595 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 129.8641 to 147.3716 deg, Dec +16.4979 to +27.3180 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 129.8641 to 147.3716 deg, Dec 16.4979 to 27.3180 deg
Loaded 5800 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): 4255 out of 4779 total matches.
Matched with Tycho-2 4779 out of 46595 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.803264
a=0.000000 b=1.000000 c=22.803264
From vast_summary.log: estimated ref. image limiting mag.: -7.32
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.48
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.48
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 111 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.4 pix Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
2.1 pix Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
2.7 pix fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits
2.8 pix fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits
Limiting magnitude estimates:
15.5 mag. Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
15.5 mag. Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
15.3 mag. fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits
15.3 mag. fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits
All-image limiting magnitude estimate: 15.3 (SNR ) 14.5 (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.MZQqGy1Ha2 (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_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits' -> 'wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
WCS_IMAGE_NAME=wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
WCS-calibrated image found: wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
Checking if the catalog wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat corresponding to the image wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits alredy exist and is non-empty...
Catalog wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat corresponding to the image wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
WCS catalog name: wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=22, blended=2637, passed=46573
Got 46573 stars (including 43885 good ones) from the SExtractor catalog wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat
util/solve_plate_with_UCAC5 got 46573 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
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: 957 matched stars entering correct_measured_positions(), 946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 45928 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
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: 957 matched stars entering correct_measured_positions(), 45926 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 45926 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits -region wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.pbK6B3P0sL (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_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits' -> 'wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
WCS_IMAGE_NAME=wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
WCS-calibrated image found: wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
Checking if the catalog wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits.cat corresponding to the image wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits alredy exist and is non-empty...
Catalog wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits.cat corresponding to the image wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
WCS catalog name: wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=2639, passed=48659
Got 48659 stars (including 45945 good ones) from the SExtractor catalog wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits.cat
util/solve_plate_with_UCAC5 got 48659 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 48061 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 48058 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 48058 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits -region wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.80P1rRYEnz (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_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.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_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits
WCS-calibrated image found: wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits
Checking if the catalog wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits.cat corresponding to the image wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits.cat corresponding to the image wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits
WCS catalog name: wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=4061, passed=38250
Got 38250 stars (including 34155 good ones) from the SExtractor catalog wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits.cat
util/solve_plate_with_UCAC5 got 38250 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.8'
Seting catalog search parameters based on the expected field of view 936.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013011 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010409 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 950 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 940 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 37432 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 950 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 37430 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 37430 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 950 stars left (next iteration limit 1045)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits -region wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.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.ByvP3dIiRN (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_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.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_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits
WCS-calibrated image found: wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits
Checking if the catalog wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits.cat corresponding to the image wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits.cat corresponding to the image wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits
WCS catalog name: wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=3771, passed=37800
Got 37800 stars (including 34003 good ones) from the SExtractor catalog wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits.cat
util/solve_plate_with_UCAC5 got 37800 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.8'
Seting catalog search parameters based on the expected field of view 936.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013011 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010409 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 941 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 37113 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 37112 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 37112 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits -region wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/wcs_Cnc-03-Q2b1x1_2026-03-19_23-13-52_20.00sec_-14.90C_LIGHT_0144.fits
Saving fully-calibrated image wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/wcs_Cnc-03-Q2b1x1_2026-03-19_23-14-46_20.00sec_-15.00C_LIGHT_0145.fits
Saving fully-calibrated image wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.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_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-44-25_20.00sec_-5.00C_LIGHT_0148.fits
Saving fully-calibrated image wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.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_2026-04-15_CI_Cnc-03-Q2b1x1_234646_TTUQ2b1x1_5685_HMANCScI/wcs_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149.fits
Preparing the HTML report for the field Cnc-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out41543.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53426.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53433.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53551.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53652.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53879.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53981.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53985.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53998.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54018.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54042.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54080.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54088.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54102.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54139.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54147.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out53731.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53775.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53808.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53838.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54365.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 16s
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
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Considering the candidate 53426_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53426_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 09:20:05.28 +19:20:11.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.63, MAG_FAINT_SEARCH_LIMIT=15.61)GAIADR2_OUTPUT=# 4.079 635741510126181120 140.02300760761 +19.33719977630 15.0483 14.4726 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.079#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53433_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53433_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 09:41:41.93 +21:20:57.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 2.397 640683574374870912 145.42400282549 +21.34946780108 14.5180 14.3792 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.397#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53434_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53434_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 09:34:50.61 +24:27:09.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53437_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53437_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 09:18:15.48 +18:23:09.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53467_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53467_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 53497_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53497_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 53551_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53551_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 09:42:10.87 +18:51:23.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 0.678 633459439382721280 145.54515438444 +18.85636349341 12.7917 12.3586 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.678#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53579_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53579_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
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Considering the candidate 53615_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53615_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 53616_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53616_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 09:42:15.68 +24:29:19.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53641_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53641_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 09:20:35.05 +22:39:16.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53643_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53643_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 09:10:55.78 +18:54:57.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53652_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53652_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 09:35:28.73 +18:24:02.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 1.172 632997399685760384 143.86996055519 +18.40080396679 13.6590 13.1351 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.172#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53654_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53654_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 09:33:48.46 +22:36:46.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53656_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53656_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 09:42:52.83 +17:53:12.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53668_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53668_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 09:35:49.57 +18:04:45.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53669_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53669_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 53672_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53672_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 53682_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53682_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 53690_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53690_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
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Considering the candidate 53691_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53691_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 09:36:06.77 +24:56:56.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53702_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53702_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 53704_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53704_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 09:37:11.20 +21:24:18.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53706_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53706_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 09:24:28.52 +19:04:52.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53708_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53708_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
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Considering the candidate 53713_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53713_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 53717_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53717_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
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Considering the candidate 53720_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53720_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 09:44:01.64 +25:18:51.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53723_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53723_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 09:38:35.96 +19:25:42.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53725_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53725_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
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Considering the candidate 53731_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
Preparing report for the candidate 53731_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
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Considering the candidate 53732_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53732_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 53738_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53738_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (16.4") between the two second-epoch detections
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Considering the candidate 53746_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53746_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 53749_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53749_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 53752_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53752_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 53756_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53756_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (16.4") between the two second-epoch detections
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Considering the candidate 53760_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53760_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 53761_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53761_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 53766_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53766_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 53774_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53774_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 53775_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
Preparing report for the candidate 53775_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
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Considering the candidate 53784_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53784_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
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Considering the candidate 53785_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53785_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 09:31:11.60 +21:09:24.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53786_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53786_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 09:18:59.75 +19:06:23.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53796_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53796_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 09:35:51.89 +19:36:13.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53799_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53799_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 53800_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53800_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 53808_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
Preparing report for the candidate 53808_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
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Considering the candidate 53810_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53810_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (16.9") between the two second-epoch detections
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Considering the candidate 53811_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53811_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (16.6") between the two second-epoch detections
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Considering the candidate 53813_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53813_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
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Considering the candidate 53816_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53816_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 53829_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53829_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
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Considering the candidate 53838_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
Preparing report for the candidate 53838_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
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Considering the candidate 53845_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53845_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
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Considering the candidate 53855_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53855_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 09:24:17.28 +20:33:58.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53860_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53860_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 09:17:52.14 +25:59:44.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53868_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53868_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (16.9") between the two second-epoch detections
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Considering the candidate 53870_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53870_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 08:57:29.91 +21:22:09.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53879_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53879_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 09:28:38.11 +21:32:47.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.45, MAG_FAINT_SEARCH_LIMIT=15.43)GAIADR2_OUTPUT=# 0.990 637931015733922304 142.15904777881 +21.54650134819 14.4826 13.8694 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.990#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53883_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53883_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 53886_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53886_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
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Considering the candidate 53888_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53888_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (16.9") between the two second-epoch detections
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Considering the candidate 53890_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53890_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 53891_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53891_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (16.9") between the two second-epoch detections
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Considering the candidate 53906_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53906_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
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Considering the candidate 53910_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53910_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (16.9") between the two second-epoch detections
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Considering the candidate 53913_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53913_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 09:40:52.62 +18:11:25.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53914_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53914_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
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Considering the candidate 53920_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53920_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 09:42:00.69 +19:35:35.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53927_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53927_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (16.9") between the two second-epoch detections
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Considering the candidate 53931_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53931_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 53936_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53936_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 09:37:57.41 +24:47:48.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53947_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53947_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
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Considering the candidate 53955_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53955_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 09:42:35.55 +19:13:35.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53956_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53956_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 09:37:20.61 +17:47:59.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53962_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53962_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 09:23:08.15 +18:12:00.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53965_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53965_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 53973_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53973_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
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Considering the candidate 53976_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53976_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (16.4") between the two second-epoch detections
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Considering the candidate 53981_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53981_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 09:38:07.39 +19:21:33.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.99, MAG_FAINT_SEARCH_LIMIT=15.97)GAIADR2_OUTPUT=# 0.579 633642508068736640 144.53085526222 +19.35918423050 14.8567 14.1291 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 53985_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53985_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 09:42:10.73 +21:00:51.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.94, MAG_FAINT_SEARCH_LIMIT=15.92)GAIADR2_OUTPUT=# 1.415 639906528891620992 145.54511433229 +21.01409056599 15.0168 14.5256 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.415#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53988_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53988_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 09:21:20.50 +19:25:26.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53990_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53990_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
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Considering the candidate 53991_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53991_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 09:39:49.63 +21:30:31.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53997_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53997_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 09:37:38.35 +19:07:04.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53998_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 53998_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 09:42:18.56 +18:21:42.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.85, MAG_FAINT_SEARCH_LIMIT=15.83)GAIADR2_OUTPUT=# 4.039 621324434489486464 145.57846219059 +18.36141740539 13.9713 12.7660 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.039#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54006_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 54006_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (16.9") between the two second-epoch detections
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Considering the candidate 54007_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 54007_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
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Considering the candidate 54018_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 54018_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 09:41:37.88 +21:12:14.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.95, MAG_FAINT_SEARCH_LIMIT=15.93)
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Considering the candidate 54032_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 54032_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
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Considering the candidate 54034_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 54034_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 09:34:27.32 +18:13:21.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54037_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 54037_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 09:18:36.71 +18:38:56.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54042_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 54042_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 09:33:15.64 +17:57:27.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.95, MAG_FAINT_SEARCH_LIMIT=15.93)GAIADR2_OUTPUT=# 1.298 632886078428551552 143.31534920258 +17.95732303759 15.1144 14.5171 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.298#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54061_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 54061_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 09:31:50.47 +18:29:18.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54068_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 54068_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (16.6") between the two second-epoch detections
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Considering the candidate 54080_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 54080_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 09:29:10.66 +18:26:20.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.85, MAG_FAINT_SEARCH_LIMIT=15.83)GAIADR2_OUTPUT=# 1.701 633140546650867840 142.29475741027 +18.43857195090 14.6796 13.7948 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.701#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54088_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 54088_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 09:19:24.34 +20:32:03.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.85, MAG_FAINT_SEARCH_LIMIT=15.83)GAIADR2_OUTPUT=# 1.804 637571750309595136 139.85157506820 +20.53467300389 15.1790 14.5650 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.804#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54090_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 54090_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
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Considering the candidate 54099_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 54099_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 54102_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 54102_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 09:32:36.57 +22:36:01.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.97, MAG_FAINT_SEARCH_LIMIT=15.95)GAIADR2_OUTPUT=# 1.077 644092507097266432 143.15268874147 +22.60043568633 14.9305 14.1895 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.077#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54131_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 54131_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
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Considering the candidate 54139_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 54139_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 09:21:09.74 +18:51:10.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.98, MAG_FAINT_SEARCH_LIMIT=15.96)GAIADR2_OUTPUT=# 2.399 632700050510076416 140.29120983505 +18.85322087073 14.9124 14.1824 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.399#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54147_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 54147_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
**** FOUND 09:15:01.00 +18:11:09.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.87, MAG_FAINT_SEARCH_LIMIT=15.85)GAIADR2_OUTPUT=# 2.352 635203638486327296 138.75460488622 +18.18636456234 14.7504 13.9475 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.352#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54153_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 54153_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 54156_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 54156_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
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Considering the candidate 54168_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 54168_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
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Considering the candidate 54227_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 54227_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 54365_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
Preparing report for the candidate 54365_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
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Considering the candidate 41543_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149
The candidate 41543_fd_Cnc-03-Q2b1x1_2026-04-15_23-45-12_20.00sec_-5.00C_LIGHT_0149 did not pass the final checks