This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY
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 14.1784* 09 36 03.75 +26 11 49.7 14.1 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,2461144.6784,14.07,0.05,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 20260414.1784 14.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461144.6784,14.23,0.05,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 20260414.1784 14.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 14.1784* 09 28 21.79 +24 20 41.2 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,2461144.6784,14.38,0.05,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 20260414.1784 14.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461144.6784,14.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260414.1784 14.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## 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: 2461144.67868561 14.04.2026 04:17:08.437 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.60
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): 6567
Objects passed selection criteria: 6562
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 6159
Average stars matched: 6065.75 (98.486 %)
Memory usage VmPeak: 113052 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 13 23:19:29 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: 2461144.67868561 14.04.2026 04:17:08.437 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 104
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: 12 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): 35615
Objects passed selection criteria: 35532
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: 33512
Average stars matched: 32182.8 (96.0335 %)
Memory usage VmPeak: 139296 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 13 23:20:13 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_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.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_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461144.67807830
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_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits exists and is non-empty
Saving wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits to local_wcs_cache/
'wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits' -> 'local_wcs_cache/wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits'
wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits exists and is non-empty
Saving wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits to local_wcs_cache/
'wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits' -> 'local_wcs_cache/wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits'
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# 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 09:14:03.197 +21:56:54.49
Angular distance between the image centers 0.0873 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:14:05.815 +22:02:06.51
Second-epoch image center 09:14:03.643 +21:57:09.68
Angular distance between the image centers 0.0829 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 09:14:03.197 +21:56:54.49
Second-epoch second image center 09:14:03.643 +21:57:09.68
Angular distance between the image centers 0.00456 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.mAJ2WJdgU9
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.yPrhHGKqKG
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_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits &> /tmp/tmp.o0AV3BvA5I
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits &> /tmp/tmp.MDef6HVCBN
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.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 2 candidate transients before the final filtering. (Hard limit: 3000)
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
2.5 pix fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits
2.4 pix fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.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_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits
15.1 mag. fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 12.2 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.mAJ2WJdgU9 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/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.yPrhHGKqKG (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/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.o0AV3BvA5I (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits
WCS-calibrated image found: wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits
Checking if the catalog wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits.cat corresponding to the image wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits.cat corresponding to the image wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.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_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits
WCS catalog name: wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=459, passed=7768
Got 7768 stars (including 7302 good ones) from the SExtractor catalog wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits.cat
util/solve_plate_with_UCAC5 got 7768 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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 16.4 to 27.2)
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 931 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 7630 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
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 16.4 to 27.2)
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 7634 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 7634 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 951 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits -region wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.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.MDef6HVCBN (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits
WCS-calibrated image found: wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits
Checking if the catalog wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits.cat corresponding to the image wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits.cat corresponding to the image wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.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_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits
WCS catalog name: wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=380, passed=6753
Got 6753 stars (including 6367 good ones) from the SExtractor catalog wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits.cat
util/solve_plate_with_UCAC5 got 6753 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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 16.4 to 27.2)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 922 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 6563 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 16.4 to 27.2)
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 6564 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 6564 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 945 stars left (next iteration limit 1039)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits -region wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.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_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/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_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/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_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits'
Saving fully-calibrated image wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits'
Preparing the HTML report for the field Cnc-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20315.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 20254_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 20254_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
**** FOUND 09:43:25.35 +19:51:41.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20315_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 20315_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
**** FOUND 09:29:31.03 +18:17:11.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 0.703 633135250955836800 142.37949737749 +18.28649844192 12.4221 11.9054 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.703#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_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.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_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.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_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.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_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits exists and is non-empty
wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits exists and is non-empty
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# 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 09:14:03.197 +21:56:54.49
Angular distance between the image centers 0.0873 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:14:05.815 +22:02:06.51
Second-epoch image center 09:14:03.643 +21:57:09.68
Angular distance between the image centers 0.0829 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 09:14:03.197 +21:56:54.49
Second-epoch second image center 09:14:03.643 +21:57:09.68
Angular distance between the image centers 0.00456 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.rrIMlKiinp
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.6oY2UbYDHm
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_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits &> /tmp/tmp.GidNUlWQKY
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits &> /tmp/tmp.LQyrRuej5x
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.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 60 candidate transients before the final filtering. (Hard limit: 3000)
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
2.3 pix fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits
2.3 pix fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.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_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits
15.3 mag. fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits
All-image limiting magnitude estimate: 15.3 (SNR ) 14.6 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.rrIMlKiinp (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/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.6oY2UbYDHm (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/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.GidNUlWQKY (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits
WCS-calibrated image found: wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits
Checking if the catalog wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits.cat corresponding to the image wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits.cat corresponding to the image wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.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_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits
WCS catalog name: wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=2221, passed=39016
Got 39016 stars (including 36747 good ones) from the SExtractor catalog wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits.cat
util/solve_plate_with_UCAC5 got 39016 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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 16.4 to 27.2)
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 933 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 38339 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
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 16.4 to 27.2)
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 38337 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 38337 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 951 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits -region wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.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.LQyrRuej5x (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits
WCS-calibrated image found: wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits
Checking if the catalog wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits.cat corresponding to the image wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits.cat corresponding to the image wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.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_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits
WCS catalog name: wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=1893, passed=35619
Got 35619 stars (including 33680 good ones) from the SExtractor catalog wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits.cat
util/solve_plate_with_UCAC5 got 35619 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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 16.4 to 27.2)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 925 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 34807 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 16.4 to 27.2)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 34806 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 34805 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 947 stars left (next iteration limit 1041)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits -region wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.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_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/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_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/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_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-16-15_20.00sec_-5.00C_LIGHT_0740.fits
Saving fully-calibrated image wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Cnc-03-Q2b1x1_231757_TTUQ2b1x1_3514_gHCo6jrY/wcs_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741.fits
Preparing the HTML report for the field Cnc-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out53697.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53775.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53785.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53791.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53809.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53846.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53866.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53906.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53943.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53945.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53957.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53996.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54005.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54028.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54040.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54089.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out53787.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53818.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53828.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53922.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 53437_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53437_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
**** FOUND 09:23:40.22 +25:32:31.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53441_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53441_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
**** FOUND 09:31:32.23 +18:32:00.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53444_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53444_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
**** FOUND 09:20:45.82 +22:04:34.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53447_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53447_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
**** FOUND 09:28:01.32 +23:18:11.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53448_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53448_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
**** FOUND 09:17:55.41 +20:03:05.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53449_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53449_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
**** FOUND 09:16:17.71 +18:22:03.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53450_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53450_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
**** FOUND 09:25:14.50 +18:45:01.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53451_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53451_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
**** FOUND 09:18:15.48 +18:23:11.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53514_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53514_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
Rejecting candidate due to large distance (15.9") between the two second-epoch detections
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Considering the candidate 53558_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53558_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 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 53560_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53560_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
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Considering the candidate 53652_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53652_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
**** FOUND 09:42:15.71 +24:29:18.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53661_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53661_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
**** FOUND 09:10:55.81 +18:54:57.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53671_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53671_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 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 53678_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53678_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 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 53680_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53680_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
**** FOUND 09:16:16.48 +23:25:02.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53697_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53697_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
**** FOUND 09:42:52.85 +17:53:12.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 0.815 621226238652521728 145.71997105402 +17.88676668450 13.6954 13.1907 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.815#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53698_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53698_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
**** FOUND 09:35:49.50 +18:04:44.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53700_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53700_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
**** FOUND 09:33:48.45 +22:36:46.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53717_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53717_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
**** FOUND 09:12:47.99 +20:01:54.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53725_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53725_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
**** FOUND 09:36:06.79 +24:56:56.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53729_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53729_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
**** FOUND 09:44:01.69 +25:18:51.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53733_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53733_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
**** FOUND 09:22:54.82 +21:56:33.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53741_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53741_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 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 53742_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53742_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
**** FOUND 09:37:11.13 +21:24:17.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53745_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53745_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
**** FOUND 09:24:28.52 +19:04:52.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53750_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53750_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
**** FOUND 09:38:35.86 +19:25:43.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53775_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53775_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
**** FOUND 09:38:35.79 +19:00:38.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 0.743 633418448214778496 144.64922486090 +19.01045526959 14.1838 13.7511 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.743#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53785_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53785_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
**** FOUND 09:24:47.50 +17:42:09.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.22, MAG_FAINT_SEARCH_LIMIT=15.20)GAIADR2_OUTPUT=# 2.487 632339032739143424 141.19847133141 +17.70230511317 14.3298 13.7056 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.487#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53787_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
Preparing report for the candidate 53787_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
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Considering the candidate 53791_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53791_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
**** FOUND 09:35:51.95 +19:36:12.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.36, MAG_FAINT_SEARCH_LIMIT=15.34)GAIADR2_OUTPUT=# 2.668 633688000362304640 143.96567981985 +19.60352241919 14.5016 13.9946 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.668#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53794_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53794_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
**** FOUND 09:18:59.73 +19:06:22.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53809_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53809_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
**** FOUND 09:25:38.41 +18:32:14.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)GAIADR2_OUTPUT=# 0.362 632453935999138048 141.41010280371 +18.53716773299 14.2451 13.7793 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.362#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53818_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
Preparing report for the candidate 53818_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
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Considering the candidate 53822_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53822_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
**** FOUND 09:11:13.89 +18:40:40.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53823_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53823_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 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 53828_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
Preparing report for the candidate 53828_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
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Considering the candidate 53846_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53846_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
**** FOUND 09:21:04.03 +19:10:48.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.57, MAG_FAINT_SEARCH_LIMIT=15.55)GAIADR2_OUTPUT=# 0.399 635746492288235776 140.26677122477 +19.18013678531 14.4644 13.9037 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.399#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53851_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53851_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
**** FOUND 08:57:29.96 +21:22:14.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53863_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53863_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
**** FOUND 09:24:17.25 +20:33:58.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53866_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53866_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
**** FOUND 09:23:03.03 +19:09:24.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)GAIADR2_OUTPUT=# 1.179 632734517622979712 140.76235512675 +19.15695571412 13.9718 12.8733 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.179#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53891_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53891_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
**** FOUND 09:21:20.40 +19:25:28.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53902_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53902_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
Rejecting candidate due to large distance (16.2") between the two second-epoch detections
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Considering the candidate 53906_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53906_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
**** FOUND 09:31:37.89 +18:48:35.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.60, MAG_FAINT_SEARCH_LIMIT=15.58)GAIADR2_OUTPUT=# 2.731 633267986920483328 142.90826699832 +18.80922723701 14.6322 14.1209 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.731#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53911_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53911_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
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Considering the candidate 53920_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53920_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
**** FOUND 09:06:09.23 +17:40:37.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53922_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
Preparing report for the candidate 53922_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
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Considering the candidate 53943_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53943_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
**** FOUND 09:40:52.64 +18:11:24.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.81, MAG_FAINT_SEARCH_LIMIT=15.79)GAIADR2_OUTPUT=# 1.150 621300009010780032 145.21949893000 +18.19041704151 14.5298 13.9056 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.150#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53944_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53944_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
**** FOUND 09:37:57.41 +24:47:47.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53945_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53945_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
**** FOUND 09:37:20.58 +17:47:58.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.95, MAG_FAINT_SEARCH_LIMIT=15.93)GAIADR2_OUTPUT=# 0.882 632905732198938112 144.33599274351 +17.79966500103 14.8306 14.3385 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.882#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53957_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53957_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
**** FOUND 09:42:35.32 +19:13:36.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=15.00, MAG_FAINT_SEARCH_LIMIT=15.98)GAIADR2_OUTPUT=# 1.124 633476275654499456 145.64748858118 +19.22679333554 14.9101 14.3438 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.124#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53963_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53963_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
**** FOUND 09:35:45.76 +18:08:59.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53976_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53976_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
**** FOUND 09:31:50.33 +18:29:20.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53983_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53983_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
**** FOUND 09:42:00.71 +19:35:36.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53996_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 53996_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
**** FOUND 09:40:58.22 +19:19:32.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.98, MAG_FAINT_SEARCH_LIMIT=15.96)GAIADR2_OUTPUT=# 0.666 633533518978634752 145.24243835887 +19.32592998696 14.9004 14.4742 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.666#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54005_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 54005_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
**** FOUND 09:40:33.50 +17:49:56.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.97, MAG_FAINT_SEARCH_LIMIT=15.95)GAIADR2_OUTPUT=# 1.217 620862811404541312 145.13991954590 +17.83233532319 14.7387 14.2421 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.217#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54028_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 54028_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
**** FOUND 09:37:38.31 +19:07:04.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.88, MAG_FAINT_SEARCH_LIMIT=15.86)GAIADR2_OUTPUT=# 0.258 633611378145782784 144.40968692818 +19.11795875967 14.7612 14.2680 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.258#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54040_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 54040_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
**** FOUND 09:32:04.73 +19:55:54.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=15.00, MAG_FAINT_SEARCH_LIMIT=15.98)GAIADR2_OUTPUT=# 1.273 634520193225962240 143.02006336120 +19.93189451845 14.7464 14.0472 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.273#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54064_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 54064_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks
**** FOUND 09:39:49.66 +21:30:30.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54089_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741
The candidate 54089_fd_Cnc-03-Q2b1x1_2026-04-13_23-17-08_20.00sec_-4.90C_LIGHT_0741 did not pass the final checks