This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
LT Hya,2461139.7930,11.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
LT Hya 20260409.2930 11.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461139.7930,11.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260409.2930 11.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461139.7930,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260409.2930 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461119.84628253 20.03.2026 08:18:28.811 /data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits
First image: 2461119.84628253 20.03.2026 08:18:28.811 /data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits
Last image: 2461139.79340711 09.04.2026 07:02:20.374 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.50
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 5695
Objects passed selection criteria: 5692
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: 5391.75
Average stars matched: 5266.5 (97.677 %)
Memory usage VmPeak: 112104 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 9 02:25:50 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461119.84628253 20.03.2026 08:18:28.811 /data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits
First image: 2461119.84628253 20.03.2026 08:18:28.811 /data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits
Last image: 2461139.79340711 09.04.2026 07:02:20.374 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 70
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.17
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: 14 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): 42126
Objects passed selection criteria: 42073
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 38794.8
Average stars matched: 37337.8 (96.2443 %)
Memory usage VmPeak: 145644 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 9 02:26:42 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits /data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits
SExtractor catalog cache: saved Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits.cat to cache
SExtractor catalog cache: saved Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.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/Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits /data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.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: 2461139.79267753
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits exists and is non-empty
Saving wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits to local_wcs_cache/
'wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits' -> 'local_wcs_cache/wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits'
wcs_Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits exists and is non-empty
Saving wcs_Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits to local_wcs_cache/
'wcs_Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits' -> 'local_wcs_cache/wcs_Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits'
wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits exists and is non-empty
Saving wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits to local_wcs_cache/
'wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits' -> 'local_wcs_cache/wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits'
wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits exists and is non-empty
Saving wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits to local_wcs_cache/
'wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits' -> 'local_wcs_cache/wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits'
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 14:36:31.344 -34:00:21.06
Second-epoch image center 14:36:40.846 -34:00:52.10
Angular distance between the image centers 0.0339 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 14:36:31.344 -34:00:21.06
Second-epoch image center 14:36:37.853 -34:00:31.14
Angular distance between the image centers 0.0227 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 14:36:40.846 -34:00:52.10
Second-epoch second image center 14:36:37.853 -34:00:31.14
Angular distance between the image centers 0.01186 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/Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits &> /tmp/tmp.TELrOpPCnE
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits &> /tmp/tmp.VXSUoQeN2D
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits &> /tmp/tmp.AhBZgpx1cF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits &> /tmp/tmp.SZfzNWcwlK
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits
Calibrating the magnitude scale
Found non-empty wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.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_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits and wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.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_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits and wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits.cat
Found non-empty wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits and wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits.cat
The reference image (wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits) and catalog (wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits.cat) found
'wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits.cat' -> 'wcsmag.cat'
Read 7514 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 209.0531 to 229.0559 deg, Dec -39.2837 to -28.4154 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 209.0531 to 229.0559 deg, Dec -39.2837 to -28.4154 deg
Loaded 10868 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 6067 out of 6192 total matches.
Matched with Tycho-2 6192 out of 7514 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.667632
a=0.000000 b=1.000000 c=22.667632
From vast_summary.log: estimated ref. image limiting mag.: -8.50
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.17
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.17
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.5 pix Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits
2.5 pix Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits
3.1 pix fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits
3.1 pix fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits
Limiting magnitude estimates:
14.2 mag. Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits
14.2 mag. Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits
13.8 mag. fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits
13.9 mag. fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 11.2 (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.TELrOpPCnE (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits' -> 'wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits
WCS_IMAGE_NAME=wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits
WCS-calibrated image found: wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits
Checking if the catalog wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits.cat corresponding to the image wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits alredy exist and is non-empty...
Catalog wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits.cat corresponding to the image wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits
WCS catalog name: wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=437, passed=7514
Got 7514 stars (including 7071 good ones) from the SExtractor catalog wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits.cat
util/solve_plate_with_UCAC5 got 7514 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.4)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 943 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 7428 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.4)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 7428 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 7428 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 950 stars left (next iteration limit 1045)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits -region wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.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.VXSUoQeN2D (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits' -> 'wcs_Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits
WCS_IMAGE_NAME=wcs_Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits
WCS-calibrated image found: wcs_Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits
Checking if the catalog wcs_Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits.cat corresponding to the image wcs_Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits alredy exist and is non-empty...
Catalog wcs_Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits.cat corresponding to the image wcs_Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits
WCS catalog name: wcs_Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=463, passed=7504
Got 7504 stars (including 7035 good ones) from the SExtractor catalog wcs_Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits.cat
util/solve_plate_with_UCAC5 got 7504 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.4)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 942 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 7391 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.4)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 7391 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 7390 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 953 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits -region wcs_Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.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.AhBZgpx1cF (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits
WCS_IMAGE_NAME=wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits
WCS-calibrated image found: wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits
Checking if the catalog wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits.cat corresponding to the image wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits alredy exist and is non-empty...
Catalog wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits.cat corresponding to the image wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits
WCS catalog name: wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=389, passed=6284
Got 6284 stars (including 5893 good ones) from the SExtractor catalog wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits.cat
util/solve_plate_with_UCAC5 got 6284 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.4)
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 939 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 6205 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.4)
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 6204 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 6204 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits -region wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.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.SZfzNWcwlK (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits
WCS_IMAGE_NAME=wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits
WCS-calibrated image found: wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits
Checking if the catalog wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits.cat corresponding to the image wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits alredy exist and is non-empty...
Catalog wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits.cat corresponding to the image wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits
WCS catalog name: wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=427, passed=6293
Got 6293 stars (including 5862 good ones) from the SExtractor catalog wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits.cat
util/solve_plate_with_UCAC5 got 6293 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.4)
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 6195 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 309 (Dec -39.3 to -28.4)
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 6194 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 6194 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits -region wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.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_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits'
Saving fully-calibrated image wcs_Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/wcs_Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits'
Saving fully-calibrated image wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits'
Saving fully-calibrated image wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits'
Preparing the HTML report for the field Cen-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20376.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20399.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out20392.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 4s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20371_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 20371_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:07:17.41 -33:12:08.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20376_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 20376_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:20:30.73 -34:59:02.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.13, MAG_FAINT_SEARCH_LIMIT=12.11)GAIADR2_OUTPUT=# 1.608 6119723218729137664 215.12756386973 -34.98370133364 9.9959 8.5912 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.608#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20392_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
Preparing report for the candidate 20392_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20399_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 20399_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:33:43.84 -36:40:16.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.36, MAG_FAINT_SEARCH_LIMIT=12.34)GAIADR2_OUTPUT=# 0.715 6118740568872082688 218.43242882095 -36.67127700655 10.4099 9.0743 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.715#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: 5s
Prepared the HTML report for the field Cen-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
14:13:33.00 -29:54:22.2
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits /data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits
SExtractor catalog cache: saved Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits.cat to cache
SExtractor catalog cache: saved Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits /data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits
Creating symlink local_wcs_cache/wcs_Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits
Creating symlink local_wcs_cache/wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits
Creating symlink local_wcs_cache/wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.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_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits exists and is non-empty
wcs_Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits exists and is non-empty
wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits exists and is non-empty
wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits exists and is non-empty
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 14:36:31.344 -34:00:21.06
Second-epoch image center 14:36:40.846 -34:00:52.10
Angular distance between the image centers 0.0339 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 14:36:31.344 -34:00:21.06
Second-epoch image center 14:36:37.853 -34:00:31.14
Angular distance between the image centers 0.0227 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 14:36:40.846 -34:00:52.10
Second-epoch second image center 14:36:37.853 -34:00:31.14
Angular distance between the image centers 0.01186 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/Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits &> /tmp/tmp.VobjJVTCEt
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits &> /tmp/tmp.xTQgd3NZVX
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits &> /tmp/tmp.hM1RORCKEf
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits &> /tmp/tmp.ykIfh4mneG
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits
Calibrating the magnitude scale
Found non-empty wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.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_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits and wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.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_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits and wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits.cat
Found non-empty wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits and wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits.cat
The reference image (wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits) and catalog (wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits.cat) found
'wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits.cat' -> 'wcsmag.cat'
Read 53362 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 209.0159 to 229.0559 deg, Dec -39.2911 to -28.3507 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 209.0159 to 229.0559 deg, Dec -39.2911 to -28.3507 deg
Loaded 10940 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 8534 out of 9205 total matches.
Matched with Tycho-2 9205 out of 53362 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.450803
a=0.000000 b=1.000000 c=22.450803
From vast_summary.log: estimated ref. image limiting mag.: -8.17
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.28
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.28
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 51 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits
2.4 pix Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits
2.8 pix fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits
2.7 pix fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits
Limiting magnitude estimates:
14.3 mag. Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits
14.3 mag. Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits
14.0 mag. fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits
14.0 mag. fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 13.4 (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.VobjJVTCEt (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits' -> 'wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits
WCS_IMAGE_NAME=wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits
WCS-calibrated image found: wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits
Checking if the catalog wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits.cat corresponding to the image wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits alredy exist and is non-empty...
Catalog wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits.cat corresponding to the image wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits
WCS catalog name: wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=2465, passed=53357
Got 53357 stars (including 50824 good ones) from the SExtractor catalog wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits.cat
util/solve_plate_with_UCAC5 got 53357 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 310 (Dec -39.3 to -28.4)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 940 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 52676 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 310 (Dec -39.3 to -28.4)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 52677 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Accuracy estimation diagnostic: 949 matched stars entering correct_measured_positions(), 52677 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 949 stars left (next iteration limit 1043)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits -region wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.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.xTQgd3NZVX (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits' -> 'wcs_Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits
WCS_IMAGE_NAME=wcs_Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits
WCS-calibrated image found: wcs_Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits
Checking if the catalog wcs_Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits.cat corresponding to the image wcs_Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits alredy exist and is non-empty...
Catalog wcs_Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits.cat corresponding to the image wcs_Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits
WCS catalog name: wcs_Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=2531, passed=54415
Got 54415 stars (including 51822 good ones) from the SExtractor catalog wcs_Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits.cat
util/solve_plate_with_UCAC5 got 54415 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 310 (Dec -39.3 to -28.4)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 942 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 53730 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 310 (Dec -39.3 to -28.4)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 53728 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 53728 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 950 stars left (next iteration limit 1045)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits -region wcs_Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.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.hM1RORCKEf (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits
WCS_IMAGE_NAME=wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits
WCS-calibrated image found: wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits
Checking if the catalog wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits.cat corresponding to the image wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits alredy exist and is non-empty...
Catalog wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits.cat corresponding to the image wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits
WCS catalog name: wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=2515, passed=39536
Got 39536 stars (including 36989 good ones) from the SExtractor catalog wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits.cat
util/solve_plate_with_UCAC5 got 39536 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 310 (Dec -39.3 to -28.4)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 934 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 39066 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 310 (Dec -39.3 to -28.4)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 39066 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 39066 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits -region wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.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.ykIfh4mneG (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits
WCS_IMAGE_NAME=wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits
WCS-calibrated image found: wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits
Checking if the catalog wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits.cat corresponding to the image wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits alredy exist and is non-empty...
Catalog wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits.cat corresponding to the image wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits
WCS catalog name: wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=2638, passed=40161
Got 40161 stars (including 37474 good ones) from the SExtractor catalog wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits.cat
util/solve_plate_with_UCAC5 got 40161 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 310 (Dec -39.3 to -28.4)
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 933 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 39583 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 310 (Dec -39.3 to -28.4)
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 39585 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 39585 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Excluding outliers - 945 stars left (next iteration limit 1039)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits -region wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.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_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits
Saving fully-calibrated image wcs_Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/wcs_Cen-03-Q2b1x1_2026-03-20_03-19-21_20.00sec_-15.00C_LIGHT_0378.fits
Saving fully-calibrated image wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-01-17_20.00sec_-5.00C_LIGHT_0252.fits
Saving fully-calibrated image wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cen-03-Q2b1x1_022338_TTUQ2b1x1_26204_Uqe0Muou/wcs_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253.fits
Preparing the HTML report for the field Cen-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out67561.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67571.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67576.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67583.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67622.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67779.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67782.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67902.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67910.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67950.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67958.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67968.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67971.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67983.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67991.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67995.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67998.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out68004.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out68009.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out68013.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out68018.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out68019.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out68021.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out68027.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out68028.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out68030.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out68034.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out68036.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out68040.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out68041.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out68042.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out68052.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out68058.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out68059.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out68079.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out68133.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out68344.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out67957.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out67657.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67726.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 67561_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 67561_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:24:40.52 -31:32:40.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 2.206 6219793109163804416 216.16937621921 -31.54509623297 13.7227 13.0382 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.206#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67566_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 67566_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:22:49.72 -35:54:35.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67571_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 67571_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:08:58.05 -31:05:27.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 0.937 6172766309648898432 212.24204505373 -31.09110449556 13.4922 12.9920 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.937#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67576_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 67576_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:15:56.26 -31:10:28.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 2.141 6124576432990465024 213.98436460740 -31.17512091912 13.3569 12.7856 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.141#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67583_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 67583_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:10:09.81 -30:34:06.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.29, MAG_FAINT_SEARCH_LIMIT=12.27)GAIADR2_OUTPUT=# 0.923 6172807403896171136 212.54098054665 -30.56879523896 11.0248 10.3443 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.923#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67622_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 67622_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:05:50.23 -34:11:36.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.05, MAG_FAINT_SEARCH_LIMIT=12.03)GAIADR2_OUTPUT=# 0.704 6122307350226501760 211.45936298882 -34.19314699058 10.9713 10.1417 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.704#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67657_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
Preparing report for the candidate 67657_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
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Considering the candidate 67726_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
Preparing report for the candidate 67726_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
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Considering the candidate 67770_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 67770_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:08:55.27 -30:06:01.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67779_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 67779_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:06:05.26 -31:41:07.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)GAIADR2_OUTPUT=# 0.528 6172345845233517568 211.52190325022 -31.68515938461 12.3102 11.5349 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.528#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67782_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 67782_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:20:51.99 -31:49:44.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 2.673 6123741761930501376 215.21578740662 -31.82870465716 12.5504 11.7287 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.673#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67838_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 67838_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:09:28.56 -34:52:09.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67847_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 67847_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:48:18.09 -31:24:47.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67859_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 67859_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:33:57.21 -31:40:43.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67893_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 67893_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:13:55.04 -38:06:22.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67897_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 67897_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:49:11.95 -34:00:50.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67902_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 67902_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:19:50.49 -33:14:03.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)
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Considering the candidate 67910_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 67910_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:46:25.35 -31:40:03.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.83, MAG_FAINT_SEARCH_LIMIT=13.81)GAIADR2_OUTPUT=# 1.210 6217517326262637824 221.60573816362 -31.66720561907 12.8776 12.3939 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.210#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67925_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 67925_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:30:52.58 -36:27:16.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67950_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 67950_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:16:59.52 -31:42:44.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 1.365 6124496271720755328 214.24785410371 -31.71258058359 13.2072 12.5743 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.365#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67957_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 67957_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:04:34.34 -33:57:38.8 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)
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Considering the candidate 67958_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 67958_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:20:06.75 -31:25:56.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 2.651 6124519808141768576 215.02897438543 -31.43249077581 13.7211 13.2328 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.651#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67968_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 67968_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:14:20.66 -35:30:56.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 1.720 6121148254517608576 213.58666550734 -35.51554933862 13.4208 12.9246 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.720#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67971_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 67971_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:05:56.95 -33:34:47.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)
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Considering the candidate 67979_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 67979_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:22:18.59 -34:48:32.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 67983_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 67983_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:10:01.81 -35:00:50.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 1.954 6121431554857355264 212.50802483491 -35.01431595415 13.6757 12.9438 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.954#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67991_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 67991_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:04:55.07 -32:55:46.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 1.429 6124127660447346688 211.22945420475 -32.93009127403 13.7868 13.3232 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.429#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67995_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 67995_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:05:17.92 -31:21:24.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 1.296 6172409208888135936 211.32494348560 -31.35718826846 13.7394 13.2021 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.296#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67998_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 67998_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:39:32.18 -31:38:58.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 4.393 6216822533686076160 219.88504405125 -31.64865004601 13.3135 12.6992 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.393#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 68004_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 68004_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:08:39.98 -30:29:07.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 1.010 6172869491943248384 212.16687944997 -30.48539446093 13.7868 13.1193 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.010#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 68009_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 68009_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:06:34.98 -31:31:59.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)
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Considering the candidate 68013_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 68013_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:11:42.59 -31:06:41.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 1.186 6124738164279000448 212.92775490569 -31.11165432887 13.9665 13.5940 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.186#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 68018_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 68018_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:17:58.45 -29:59:38.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 2.059 6220937151012329216 214.49398254839 -29.99456477381 13.8788 13.2721 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.059#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 68019_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 68019_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:08:04.78 -29:43:53.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 3.050 6173096815972197248 212.01970927015 -29.73230006613 13.8313 13.3497 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.050#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 68021_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 68021_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:06:14.65 -29:56:47.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 0.329 6173111143982963200 211.56114726227 -29.94663664558 13.7252 13.2528 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.329#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 68027_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 68027_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:14:07.54 -30:52:48.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 2.261 6124827980634988928 213.53143209933 -30.87937203401 13.9683 13.4643 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.261#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 68028_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 68028_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:09:14.46 -30:34:21.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 0.818 6172853407288944256 212.31045725493 -30.57264071703 13.7717 13.2223 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.818#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 68030_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 68030_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:09:58.46 -34:26:52.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 2.084 6121500033816086400 212.49408342763 -34.44843422819 13.7095 13.0514 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.084#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 68034_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 68034_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:04:53.95 -31:31:35.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 2.549 6172400584593513728 211.22454936688 -31.52726069990 13.7217 13.2358 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.549#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 68036_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 68036_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:05:22.51 -33:35:54.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 1.368 6122545497574878336 211.34389141300 -33.59799038282 13.5979 12.8939 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.368#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 68040_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 68040_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:20:15.59 -32:53:30.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 0.458 6123345151766383744 215.06498561010 -32.89156932481 14.1163 13.6484 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.458#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 68041_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 68041_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:08:41.27 -33:22:33.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 0.278 6123857214947059584 212.17188316836 -33.37598945658 13.7559 13.2712 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.278#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 68042_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 68042_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:10:53.82 -31:59:22.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 1.385 6124254306147415808 212.72396826785 -31.98939293040 13.5866 12.7832 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.385#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 68052_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 68052_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:10:00.29 -33:32:13.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 0.537 6123824397099827712 212.50137857938 -33.53712972998 13.8821 13.3933 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.537#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 68058_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 68058_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:12:40.47 -31:38:19.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 2.507 6124630923238457216 213.16879034161 -31.63948767329 13.8302 13.4112 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.507#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 68059_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 68059_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:10:37.01 -32:42:21.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 2.338 6124008603954602112 212.65345414113 -32.70599896155 13.9527 13.4692 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.338#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 68079_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 68079_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:16:02.08 -32:25:20.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 2.678 6124345260670784256 214.00839644479 -32.42318039996 13.9938 13.5277 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.678#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 68133_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 68133_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:09:30.75 -35:36:26.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 0.867 6121377678787454720 212.37840897011 -35.60723685716 13.6171 13.1163 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.867#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 68344_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 68344_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:39:58.03 -36:38:11.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 1.089 6106595638307955584 219.99212227987 -36.63658996995 14.0697 13.5594 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.089#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 48327_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 48327_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks
**** FOUND 14:46:33.35 -31:27:20.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 41386_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253
The candidate 41386_fd_Cen-03-Q2b1x1_2026-04-09_02-02-20_20.00sec_-5.00C_LIGHT_0253 did not pass the final checks