This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.9874,13.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.4874 13.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:14:51.69 +25:19:05.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20_00sec_-15_00C_LIGHT_0682_fits__*pix.png resample_wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20_00sec_-14_90C_LIGHT_0392_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20_00sec_-15_00C_LIGHT_0682_fits__*pix.png resample_wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20_00sec_-15_00C_LIGHT_0391_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20_00sec_-15_00C_LIGHT_0682_fits__*pix.png resample_wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20_00sec_-14_90C_LIGHT_0392_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20_00sec_-15_00C_LIGHT_0682_fits__*pix.png resample_wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png animation_v2.gif
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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
IY Boo,2461121.9874,13.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
IY Boo 20260322.4874 13.83CV 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
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:19:39.22 +25:47:24.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20_00sec_-15_00C_LIGHT_0682_fits__*pix.png resample_wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20_00sec_-14_90C_LIGHT_0392_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20_00sec_-15_00C_LIGHT_0682_fits__*pix.png resample_wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20_00sec_-15_00C_LIGHT_0391_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20_00sec_-15_00C_LIGHT_0682_fits__*pix.png resample_wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20_00sec_-14_90C_LIGHT_0392_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20_00sec_-15_00C_LIGHT_0682_fits__*pix.png resample_wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20_00sec_-15_00C_LIGHT_0391_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461033.01408645 23.12.2025 12:20:07.069 /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits
First image: 2461033.01408645 23.12.2025 12:20:07.069 /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits
Last image: 2461121.98759009 22.03.2026 11:41:57.784 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.49
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: 7 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): 5929
Objects passed selection criteria: 5924
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: 5531
Average stars matched: 5394 (97.5231 %)
Memory usage VmPeak: 112052 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Mar 22 06:53:27 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: 2461033.01408645 23.12.2025 12:20:07.069 /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits
First image: 2461033.01408645 23.12.2025 12:20:07.069 /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits
Last image: 2461121.98759009 22.03.2026 11:41:57.784 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 81
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.25
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: 22 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): 32608
Objects passed selection criteria: 32523
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: 30976.8
Average stars matched: 29745.8 (96.0261 %)
Memory usage VmPeak: 134156 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Mar 22 06:54:47 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits
SExtractor catalog cache: saved CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits.cat to cache
SExtractor catalog cache: saved CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.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/CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.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: 2461121.98712226
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'
Plate-solving the images
wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits exists and is non-empty
Saving wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits to local_wcs_cache/
'wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits' -> 'local_wcs_cache/wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits'
wcs_CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits exists and is non-empty
Saving wcs_CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits to local_wcs_cache/
'wcs_CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits' -> 'local_wcs_cache/wcs_CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits'
wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits exists and is non-empty
Saving wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits to local_wcs_cache/
'wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits' -> 'local_wcs_cache/wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits'
wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits exists and is non-empty
Saving wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits to local_wcs_cache/
'wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits' -> 'local_wcs_cache/wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 14:00:00.841 +29:59:53.58
Second-epoch image center 13:59:59.022 +29:59:56.30
Angular distance between the image centers 0.01 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 14:00:00.841 +29:59:53.58
Second-epoch image center 14:00:00.889 +29:59:50.79
Angular distance between the image centers 0.00 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 13:59:59.022 +29:59:56.30
Second-epoch second image center 14:00:00.889 +29:59:50.79
Angular distance between the image centers 0.00691 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/CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits &> /tmp/tmp.o9VNjGlGHm
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits &> /tmp/tmp.CjpkrCuXGH
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits &> /tmp/tmp.ZfKppU7IfZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits &> /tmp/tmp.WFlIm3P2AB
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits
Calibrating the magnitude scale
Found non-empty wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.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_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits and wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.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_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits and wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits.cat
Found non-empty wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits and wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits.cat
The reference image (wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits) and catalog (wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits.cat) found
'wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits.cat' -> 'wcsmag.cat'
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
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 3498 out of 5934 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.948197
a=0.000000 b=1.000000 c=22.948197
From vast_summary.log: estimated ref. image limiting mag.: -7.49
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.46
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.46
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits
2.1 pix CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits
2.0 pix fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits
2.0 pix fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits
Limiting magnitude estimates:
15.5 mag. CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits
15.5 mag. CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits
15.3 mag. fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits
15.3 mag. fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits
All-image limiting magnitude estimate: 15.3 (SNR ) 12.2 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.o9VNjGlGHm (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_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits' -> 'wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits
WCS_IMAGE_NAME=wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits
WCS-calibrated image found: wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits
Checking if the catalog wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits.cat corresponding to the image wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits alredy exist and is non-empty...
Catalog wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits.cat corresponding to the image wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits
WCS catalog name: wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits.cat
SExtractor catalog parsing summary: zero_flux=4, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=390, passed=5930
Got 5930 stars (including 5534 good ones) from the SExtractor catalog wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits.cat
util/solve_plate_with_UCAC5 got 5930 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.30"
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits -region wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.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.CjpkrCuXGH (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_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits' -> 'wcs_CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits
WCS_IMAGE_NAME=wcs_CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits
WCS-calibrated image found: wcs_CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits
Checking if the catalog wcs_CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits.cat corresponding to the image wcs_CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits alredy exist and is non-empty...
Catalog wcs_CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits.cat corresponding to the image wcs_CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits
WCS catalog name: wcs_CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=381, passed=5920
Got 5920 stars (including 5528 good ones) from the SExtractor catalog wcs_CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits.cat
util/solve_plate_with_UCAC5 got 5920 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.29"
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits -region wcs_CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.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.ZfKppU7IfZ (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_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.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_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits
WCS_IMAGE_NAME=wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits
WCS-calibrated image found: wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits
Checking if the catalog wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits.cat corresponding to the image wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits alredy exist and is non-empty...
Catalog wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits.cat corresponding to the image wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits
WCS catalog name: wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits.cat
SExtractor catalog parsing summary: zero_flux=4, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=357, passed=5201
Got 5201 stars (including 4839 good ones) from the SExtractor catalog wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits.cat
util/solve_plate_with_UCAC5 got 5201 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.28"
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 964 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits -region wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.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.WFlIm3P2AB (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_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.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_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits
WCS_IMAGE_NAME=wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits
WCS-calibrated image found: wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits
Checking if the catalog wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits.cat corresponding to the image wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits alredy exist and is non-empty...
Catalog wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits.cat corresponding to the image wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits
WCS catalog name: wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=362, passed=5233
Got 5233 stars (including 4864 good ones) from the SExtractor catalog wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits.cat
util/solve_plate_with_UCAC5 got 5233 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.27"
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 966 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits -region wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.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_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits'
Saving fully-calibrated image wcs_CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/wcs_CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits'
Saving fully-calibrated image wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits'
Saving fully-calibrated image wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits'
Preparing the HTML report for the field CVn-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20314.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20314_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392
The candidate 20314_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392 did not pass the final checks
**** FOUND 14:22:44.51 +24:49:43.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.82, MAG_FAINT_SEARCH_LIMIT=10.80)GAIADR2_OUTPUT=# 1.433 1255642489374284160 215.68586405424 +24.82868185109 9.6900 9.2090 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.433#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field CVn-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits
SExtractor catalog cache: saved CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits.cat to cache
SExtractor catalog cache: saved CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits
Creating symlink local_wcs_cache/wcs_CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits
Creating symlink local_wcs_cache/wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits
Creating symlink local_wcs_cache/wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.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_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits exists and is non-empty
wcs_CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits exists and is non-empty
wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits exists and is non-empty
wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 14:00:00.841 +29:59:53.58
Second-epoch image center 13:59:59.022 +29:59:56.30
Angular distance between the image centers 0.01 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 14:00:00.841 +29:59:53.58
Second-epoch image center 14:00:00.889 +29:59:50.79
Angular distance between the image centers 0.00 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 13:59:59.022 +29:59:56.30
Second-epoch second image center 14:00:00.889 +29:59:50.79
Angular distance between the image centers 0.00691 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/CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits &> /tmp/tmp.oa9DEK2rjN
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits &> /tmp/tmp.RsxppowaoF
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits &> /tmp/tmp.Ad1RLvv6Lv
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits &> /tmp/tmp.wFkWjLjrr7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits
Calibrating the magnitude scale
Found non-empty wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.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_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits and wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.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_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits and wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits.cat
Found non-empty wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits and wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits.cat
The reference image (wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits) and catalog (wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits.cat) found
'wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits.cat' -> 'wcsmag.cat'
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
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 3526 out of 32753 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.846820
a=0.000000 b=1.000000 c=22.846820
From vast_summary.log: estimated ref. image limiting mag.: -7.25
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.60
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.60
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 45 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits
2.0 pix CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits
2.0 pix fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits
2.0 pix fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits
Limiting magnitude estimates:
15.6 mag. CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits
15.6 mag. CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits
15.4 mag. fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits
15.4 mag. fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits
All-image limiting magnitude estimate: 15.4 (SNR ) 14.8 (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.oa9DEK2rjN (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_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits' -> 'wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits
WCS_IMAGE_NAME=wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits
WCS-calibrated image found: wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits
Checking if the catalog wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits.cat corresponding to the image wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits alredy exist and is non-empty...
Catalog wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits.cat corresponding to the image wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits
WCS catalog name: wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=1239, passed=32743
Got 32743 stars (including 31462 good ones) from the SExtractor catalog wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits.cat
util/solve_plate_with_UCAC5 got 32743 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.31"
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits -region wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.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.RsxppowaoF (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_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits' -> 'wcs_CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits
WCS_IMAGE_NAME=wcs_CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits
WCS-calibrated image found: wcs_CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits
Checking if the catalog wcs_CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits.cat corresponding to the image wcs_CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits alredy exist and is non-empty...
Catalog wcs_CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits.cat corresponding to the image wcs_CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits
WCS catalog name: wcs_CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=1227, passed=32749
Got 32749 stars (including 31460 good ones) from the SExtractor catalog wcs_CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits.cat
util/solve_plate_with_UCAC5 got 32749 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.31"
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits -region wcs_CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.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.Ad1RLvv6Lv (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_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.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_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits
WCS_IMAGE_NAME=wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits
WCS-calibrated image found: wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits
Checking if the catalog wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits.cat corresponding to the image wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits alredy exist and is non-empty...
Catalog wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits.cat corresponding to the image wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits
WCS catalog name: wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits.cat
SExtractor catalog parsing summary: zero_flux=2, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=1009, passed=29603
Got 29603 stars (including 28551 good ones) from the SExtractor catalog wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits.cat
util/solve_plate_with_UCAC5 got 29603 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.29"
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits -region wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.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.wFkWjLjrr7 (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_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.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_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits
WCS_IMAGE_NAME=wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits
WCS-calibrated image found: wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits
Checking if the catalog wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits.cat corresponding to the image wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits alredy exist and is non-empty...
Catalog wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits.cat corresponding to the image wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits
WCS catalog name: wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=1038, passed=29524
Got 29524 stars (including 28442 good ones) from the SExtractor catalog wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits.cat
util/solve_plate_with_UCAC5 got 29524 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.28"
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits -region wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.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_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.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_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/wcs_CVn-03-Q1b1x1_2025-12-23_06-20-07_20.00sec_-15.00C_LIGHT_0682.fits
Saving fully-calibrated image wcs_CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.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_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/wcs_CVn-03-Q1b1x1_2025-12-23_06-21-00_20.00sec_-15.00C_LIGHT_0683.fits
Saving fully-calibrated image wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.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_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-17_20.00sec_-15.00C_LIGHT_0391.fits
Saving fully-calibrated image wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.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_2026-03-22_CI_CVn-03-Q1b1x1_065113_TTUQ1b1x1_3935_4NRmUbjp/wcs_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392.fits
Preparing the HTML report for the field CVn-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out52469.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52470.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52473.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52475.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52476.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52477.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52481.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52483.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52485.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52486.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52518.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52757.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52919.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53213.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53271.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53316.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53332.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53342.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53388.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53423.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53443.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53467.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53470.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53494.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53497.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53499.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53501.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53527.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53547.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53559.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53584.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53598.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53626.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out02927.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52993.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 23s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 52469_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392
The candidate 52469_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392 did not pass the final checks
**** FOUND 14:27:49.05 +30:06:46.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.92, MAG_FAINT_SEARCH_LIMIT=15.90)GAIADR2_OUTPUT=# 1.644 1284468145201776256 216.95404240746 +30.11329907635 15.2033 14.6415 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.644#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52470_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392
The candidate 52470_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392 did not pass the final checks
**** FOUND 14:17:02.07 +29:09:46.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.93, MAG_FAINT_SEARCH_LIMIT=15.91)GAIADR2_OUTPUT=# 1.099 1260911211656028288 214.25868471985 +29.16267130908 14.8557 14.3536 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.099#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52473_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392
The candidate 52473_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392 did not pass the final checks
**** FOUND 13:48:34.78 +32:30:01.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.90, MAG_FAINT_SEARCH_LIMIT=15.88)GAIADR2_OUTPUT=# 1.102 1458205138605019392 207.14456699136 +32.50044283384 14.8301 14.1789 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.102#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52475_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392
The candidate 52475_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392 did not pass the final checks
**** FOUND 13:50:54.75 +28:34:06.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.62, MAG_FAINT_SEARCH_LIMIT=15.60)GAIADR2_OUTPUT=# 1.383 1452172771136035072 207.72821284526 +28.56798480406 14.6639 14.1031 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.383#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52476_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392
The candidate 52476_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392 did not pass the final checks
**** FOUND 14:34:26.07 +31:33:14.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.74, MAG_FAINT_SEARCH_LIMIT=15.72)GAIADR2_OUTPUT=# 1.751 1286169948683348480 218.60806484420 +31.55401001153 14.5759 13.7549 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.751#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52477_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392
The candidate 52477_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392 did not pass the final checks
**** FOUND 14:02:55.39 +25:06:08.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.53, MAG_FAINT_SEARCH_LIMIT=15.51)GAIADR2_OUTPUT=# 1.391 1258266302075301248 210.73055819987 +25.10195420468 14.7054 14.2875 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.391#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52481_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392
The candidate 52481_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392 did not pass the final checks
**** FOUND 14:36:12.83 +31:53:21.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.24, MAG_FAINT_SEARCH_LIMIT=15.22)GAIADR2_OUTPUT=# 2.584 1286273646376955008 219.05261345287 +31.88913977540 14.4625 13.9853 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.584#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52483_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392
The candidate 52483_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392 did not pass the final checks
**** FOUND 14:32:39.58 +30:05:11.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)GAIADR2_OUTPUT=# 0.452 1284325036891620224 218.16491670063 +30.08642993222 14.2576 13.7531 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.452#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52485_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392
The candidate 52485_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392 did not pass the final checks
**** FOUND 14:27:51.80 +26:54:24.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)
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Considering the candidate 52486_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392
The candidate 52486_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392 did not pass the final checks
**** FOUND 13:27:09.52 +25:33:47.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 1.589 1448197108888502528 201.79015466955 +25.56302275655 14.0951 13.5485 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.589#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52487_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392
The candidate 52487_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392 did not pass the final checks
**** FOUND 14:35:39.45 +34:23:10.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52488_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392
The candidate 52488_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392 did not pass the final checks
**** FOUND 13:49:20.32 +34:51:32.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52489_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392
The candidate 52489_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392 did not pass the final checks
**** FOUND 14:11:28.40 +33:03:03.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52490_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392
The candidate 52490_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392 did not pass the final checks
**** FOUND 14:31:32.22 +28:51:22.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52518_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392
The candidate 52518_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392 did not pass the final checks
**** FOUND 14:22:44.51 +24:49:43.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.82, MAG_FAINT_SEARCH_LIMIT=10.80)GAIADR2_OUTPUT=# 1.433 1255642489374284160 215.68586405424 +24.82868185109 9.6900 9.2090 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.433#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52736_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392
The candidate 52736_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392 did not pass the final checks
**** FOUND 13:31:07.47 +26:23:27.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52757_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392
The candidate 52757_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392 did not pass the final checks
**** FOUND 14:29:05.02 +32:55:34.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 1.708 1287292481340931584 217.27038594250 +32.92594794666 13.2432 12.7388 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.708#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52919_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392
The candidate 52919_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392 did not pass the final checks
**** FOUND 14:36:55.95 +33:11:27.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 0.202 1287490908827071104 219.23318783174 +33.19107487208 13.7294 13.1336 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.202#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52993_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392
Preparing report for the candidate 52993_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392
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Considering the candidate 53064_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392
The candidate 53064_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392 did not pass the final checks
**** FOUND 14:31:19.33 +30:54:39.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53085_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392
The candidate 53085_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392 did not pass the final checks
**** FOUND 14:11:29.86 +28:03:10.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53119_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392
The candidate 53119_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392 did not pass the final checks
**** FOUND 13:44:47.65 +25:31:35.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53213_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392
The candidate 53213_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392 did not pass the final checks
**** FOUND 14:12:44.63 +25:29:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.71, MAG_FAINT_SEARCH_LIMIT=15.69)GAIADR2_OUTPUT=# 0.620 1259047470727064832 213.18576827550 +25.49642945637 14.7139 14.2178 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.620#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53271_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392
The candidate 53271_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392 did not pass the final checks
**** FOUND 14:05:33.22 +28:32:18.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.48, MAG_FAINT_SEARCH_LIMIT=15.46)GAIADR2_OUTPUT=# 5.059 1452632229558236928 211.38954644338 +28.53739422838 14.7828 14.0966 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.059#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53316_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392
The candidate 53316_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392 did not pass the final checks
**** FOUND 14:28:08.41 +31:07:05.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.60, MAG_FAINT_SEARCH_LIMIT=15.58)GAIADR2_OUTPUT=# 0.695 1285381083450390272 217.03481869580 +31.11813805423 14.6325 14.1127 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.695#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53332_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392
The candidate 53332_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392 did not pass the final checks
**** FOUND 14:34:12.24 +31:00:15.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.78, MAG_FAINT_SEARCH_LIMIT=15.76)GAIADR2_OUTPUT=# 0.583 1286079307693460224 218.55104220642 +31.00443557915 14.7429 14.2073 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.583#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53337_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392
The candidate 53337_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392 did not pass the final checks
**** FOUND 14:34:20.00 +32:31:52.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 53342_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392
The candidate 53342_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392 did not pass the final checks
**** FOUND 14:36:45.32 +32:17:55.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.90, MAG_FAINT_SEARCH_LIMIT=15.88)GAIADR2_OUTPUT=# 1.278 1286323124400292224 219.18860689648 +32.29853446588 14.9538 14.4046 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.278#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53388_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392
The candidate 53388_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392 did not pass the final checks
**** FOUND 14:23:58.40 +33:09:15.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.91, MAG_FAINT_SEARCH_LIMIT=15.89)GAIADR2_OUTPUT=# 0.465 1478003872690093312 215.99321601848 +33.15422148183 15.0137 14.3928 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.465#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53423_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392
The candidate 53423_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392 did not pass the final checks
**** FOUND 14:25:39.98 +26:59:38.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.86, MAG_FAINT_SEARCH_LIMIT=15.84)GAIADR2_OUTPUT=# 0.647 1256493545734094848 216.41638564435 +26.99399159785 14.6231 13.8368 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.647#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53443_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392
The candidate 53443_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392 did not pass the final checks
**** FOUND 14:29:32.17 +28:40:31.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.92, MAG_FAINT_SEARCH_LIMIT=15.90)GAIADR2_OUTPUT=# 0.685 1283725631255377792 217.38382551340 +28.67543357639 15.0462 14.5136 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.685#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53467_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392
The candidate 53467_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392 did not pass the final checks
**** FOUND 14:15:18.11 +34:20:33.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.96, MAG_FAINT_SEARCH_LIMIT=15.94)GAIADR2_OUTPUT=# 1.231 1479294012142416128 213.82585903775 +34.34272535448 15.2240 14.7340 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.231#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53470_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392
The candidate 53470_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392 did not pass the final checks
**** FOUND 14:24:53.12 +27:54:54.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.81, MAG_FAINT_SEARCH_LIMIT=15.79)GAIADR2_OUTPUT=# 1.304 1283604719336026624 216.22127348210 +27.91469731773 14.8611 14.4012 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.304#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53494_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392
The candidate 53494_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392 did not pass the final checks
**** FOUND 14:28:41.30 +29:09:33.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.99, MAG_FAINT_SEARCH_LIMIT=15.97)GAIADR2_OUTPUT=# 0.687 1283804693013412736 217.17192276834 +29.15906481354 15.0517 14.4060 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.687#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53497_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392
The candidate 53497_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392 did not pass the final checks
**** FOUND 14:20:25.07 +27:59:05.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.96, MAG_FAINT_SEARCH_LIMIT=15.94)GAIADR2_OUTPUT=# 1.337 1259823691576548608 215.10404165775 +27.98502279795 14.8067 14.0960 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.337#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53499_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392
The candidate 53499_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392 did not pass the final checks
**** FOUND 14:24:28.59 +28:39:13.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.98, MAG_FAINT_SEARCH_LIMIT=15.96)GAIADR2_OUTPUT=# 1.823 1283864066641235200 216.11855079553 +28.65377239235 14.9399 14.3353 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.823#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53501_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392
The candidate 53501_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392 did not pass the final checks
**** FOUND 14:11:29.47 +27:56:26.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.95, MAG_FAINT_SEARCH_LIMIT=15.93)GAIADR2_OUTPUT=# 0.664 1260350357646316032 212.87275530112 +27.94056838089 14.9841 14.5402 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.664#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53527_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392
The candidate 53527_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392 did not pass the final checks
**** FOUND 13:35:44.19 +25:28:09.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.93, MAG_FAINT_SEARCH_LIMIT=15.91)GAIADR2_OUTPUT=# 0.302 1445061129927639040 203.93411672101 +25.46927786084 14.7160 14.1889 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.302#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53547_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392
The candidate 53547_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392 did not pass the final checks
**** FOUND 14:27:17.79 +30:41:16.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.93, MAG_FAINT_SEARCH_LIMIT=15.91)GAIADR2_OUTPUT=# 1.438 1285270238934109056 216.82382906662 +30.68825234471 15.0818 14.5219 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.438#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53559_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392
The candidate 53559_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392 did not pass the final checks
**** FOUND 14:28:16.74 +30:19:24.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.99, MAG_FAINT_SEARCH_LIMIT=15.97)GAIADR2_OUTPUT=# 1.864 1284495598632735872 217.07009481606 +30.32310399523 15.0369 14.3849 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.864#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53584_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392
The candidate 53584_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392 did not pass the final checks
**** FOUND 14:34:04.34 +29:24:50.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.90, MAG_FAINT_SEARCH_LIMIT=15.88)GAIADR2_OUTPUT=# 0.396 1284140353297796864 218.51800016402 +29.41405604275 15.0215 14.5388 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.396#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53598_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392
The candidate 53598_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392 did not pass the final checks
**** FOUND 14:26:40.39 +34:12:39.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.96, MAG_FAINT_SEARCH_LIMIT=15.94)GAIADR2_OUTPUT=# 1.023 1479666402987036288 216.66796028965 +34.21092476924 14.8560 14.3989 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.023#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53626_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392
The candidate 53626_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392 did not pass the final checks
**** FOUND 14:31:11.52 +31:50:46.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.99, MAG_FAINT_SEARCH_LIMIT=15.97)GAIADR2_OUTPUT=# 0.441 1286929470701127168 217.79812384539 +31.84625732956 15.0458 14.4628 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.441#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 02927_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392
Preparing report for the candidate 02927_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392
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Considering the candidate 14067_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392
The candidate 14067_fd_CVn-03-Q1b1x1_2026-03-22_06-41-57_20.00sec_-14.90C_LIGHT_0392 did not pass the final checks