This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461149.7664,11.31,0.05,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 20260419.2664 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461149.7664,11.80,0.05,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 20260419.2664 11.80CV 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: 2461149.76746652 19.04.2026 06:24:59.107 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 7
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -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: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 5516
Objects passed selection criteria: 5512
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 5095.75
Average stars matched: 4992.5 (97.9738 %)
Memory usage VmPeak: 112108 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Apr 19 01:29:16 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: 2461149.76746652 19.04.2026 06:24:59.107 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 47
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: 18 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 41316
Objects passed selection criteria: 41266
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 36840
Average stars matched: 35530.5 (96.4454 %)
Memory usage VmPeak: 145640 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Apr 19 01:30:25 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/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_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.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_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461149.76529365
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_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits exists and is non-empty
Saving wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits to local_wcs_cache/
'wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits' -> 'local_wcs_cache/wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits'
wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits exists and is non-empty
Saving wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits to local_wcs_cache/
'wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits' -> 'local_wcs_cache/wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits (1st reference image)
verification OK: wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits
Image size: 937.6'x625.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 14:36:31.344 -34:00:21.06 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits (1st new image)
verification OK: wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits
Image size: 937.1'x625.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 14:36:34.545 -33:59:16.86 J2000 4789.000 3195.000
###################################
###################################
# 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 14:36:34.545 -33:59:16.86
Angular distance between the image centers 0.0210 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits (2nd new image)
verification OK: wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits
Image size: 937.3'x625.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 14:36:33.027 -33:59:47.82 J2000 4789.000 3195.000
###################################
###################################
# 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 14:36:33.027 -33:59:47.82
Angular distance between the image centers 0.0109 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 14:36:34.545 -33:59:16.86
Second-epoch second image center 14:36:33.027 -33:59:47.82
Angular distance between the image centers 0.01007 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.URAPGGPRKI
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.oZTq4C953a
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_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits &> /tmp/tmp.JgHwEUsBMX
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits &> /tmp/tmp.3q3rkiKXeF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.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 5 candidate transients before the final filtering. (Hard limit: 8000)
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
3.3 pix fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits
2.8 pix fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.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
13.6 mag. fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits
13.8 mag. fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits
All-image limiting magnitude estimate: 13.6 (SNR ) 11.1 (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.URAPGGPRKI (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/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.oZTq4C953a (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/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.JgHwEUsBMX (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits
WCS_IMAGE_NAME=wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits
WCS-calibrated image found: wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits
Checking if the catalog wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits.cat corresponding to the image wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits alredy exist and is non-empty...
Catalog wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits.cat corresponding to the image wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.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_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits
WCS catalog name: wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=300, passed=5400
Got 5400 stars (including 5100 good ones) from the SExtractor catalog wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits.cat
util/solve_plate_with_UCAC5 got 5400 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 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 937 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 5326 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 309 (Dec -39.3 to -28.4)
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 5326 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 5326 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Excluding outliers - 946 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits -region wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.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.3q3rkiKXeF (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits
WCS_IMAGE_NAME=wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits
WCS-calibrated image found: wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits
Checking if the catalog wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits.cat corresponding to the image wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits alredy exist and is non-empty...
Catalog wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits.cat corresponding to the image wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.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_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits
WCS catalog name: wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=349, passed=5629
Got 5629 stars (including 5273 good ones) from the SExtractor catalog wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits.cat
util/solve_plate_with_UCAC5 got 5629 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 939 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 5542 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
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 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 5542 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 5542 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Excluding outliers - 951 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits -region wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.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_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/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_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/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_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits'
Saving fully-calibrated image wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits'
Preparing the HTML report for the field Cen-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
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 20358_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542
The candidate 20358_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542 did not pass the final checks
**** FOUND 14:13:32.99 -29:54:21.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20367_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542
The candidate 20367_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542 did not pass the final checks
**** FOUND 14:05:50.18 -34:11:36.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20370_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542
The candidate 20370_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542 did not pass the final checks
**** FOUND 14:07:17.40 -33:12:08.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20371_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542
The candidate 20371_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542 did not pass the final checks
**** FOUND 14:20:30.71 -34:59:02.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20391_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542
The candidate 20391_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542 did not pass the final checks
**** FOUND 14:41:21.95 -31:18:19.4 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
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 ####
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_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.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_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.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_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits
Creating symlink local_wcs_cache/wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.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_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits exists and is non-empty
wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits (1st reference image)
verification OK: wcs_Cen-03-Q2b1x1_2026-03-20_03-18-28_20.00sec_-15.00C_LIGHT_0377.fits
Image size: 937.6'x625.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 14:36:31.344 -34:00:21.06 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits (1st new image)
verification OK: wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits
Image size: 937.1'x625.0' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 14:36:34.545 -33:59:16.86 J2000 4789.000 3195.000
###################################
###################################
# 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 14:36:34.545 -33:59:16.86
Angular distance between the image centers 0.0210 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits (2nd new image)
verification OK: wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits
Image size: 937.3'x625.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 14:36:33.027 -33:59:47.82 J2000 4789.000 3195.000
###################################
###################################
# 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 14:36:33.027 -33:59:47.82
Angular distance between the image centers 0.0109 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 14:36:34.545 -33:59:16.86
Second-epoch second image center 14:36:33.027 -33:59:47.82
Angular distance between the image centers 0.01007 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.aBf6Pi1mne
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.l6oSoMbeIV
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_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits &> /tmp/tmp.uT2UTeQbnh
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits &> /tmp/tmp.YA450b970t
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.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 30 candidate transients before the final filtering. (Hard limit: 8000)
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
3.2 pix fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits
2.5 pix fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.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
13.8 mag. fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits
13.9 mag. fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 13.2 (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.aBf6Pi1mne (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/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.l6oSoMbeIV (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/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.uT2UTeQbnh (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits
WCS_IMAGE_NAME=wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits
WCS-calibrated image found: wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits
Checking if the catalog wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits.cat corresponding to the image wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits alredy exist and is non-empty...
Catalog wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits.cat corresponding to the image wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.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_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits
WCS catalog name: wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=1, no_mag_err=0, low_SNR=3, blended=1656, passed=31855
Got 31855 stars (including 30181 good ones) from the SExtractor catalog wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits.cat
util/solve_plate_with_UCAC5 got 31855 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 -28.3)
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(), 933 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 31505 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
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 -28.3)
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(), 31504 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Accuracy estimation diagnostic: 944 matched stars entering correct_measured_positions(), 31505 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
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_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits -region wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.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.YA450b970t (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits
WCS_IMAGE_NAME=wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits
WCS-calibrated image found: wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits
Checking if the catalog wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits.cat corresponding to the image wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits alredy exist and is non-empty...
Catalog wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits.cat corresponding to the image wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.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_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits
WCS catalog name: wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=1923, passed=38574
Got 38574 stars (including 36606 good ones) from the SExtractor catalog wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits.cat
util/solve_plate_with_UCAC5 got 38574 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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 950 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 38057 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
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 950 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 38057 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 38057 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Excluding outliers - 947 stars left (next iteration limit 1041)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits -region wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.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_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/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_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/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_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-21-51_20.00sec_-5.00C_LIGHT_0541.fits
Saving fully-calibrated image wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Cen-03-Q2b1x1_012535_TTUQ2b1x1_3979560_yOJYNCD2/wcs_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542.fits
Preparing the HTML report for the field Cen-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out67573.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67903.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67924.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67926.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67935.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67941.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67945.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out67975.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out67628.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67675.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
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 67573_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542
The candidate 67573_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542 did not pass the final checks
**** FOUND 14:27:55.25 -32:19:58.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.77, MAG_FAINT_SEARCH_LIMIT=12.75)GAIADR2_OUTPUT=# 1.854 6219508537513722624 216.98081559667 -32.33295544314 11.9636 11.2218 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.854#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67574_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542
The candidate 67574_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542 did not pass the final checks
**** FOUND 14:10:09.83 -30:34:07.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67609_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542
The candidate 67609_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542 did not pass the final checks
**** FOUND 14:05:50.24 -34:11:35.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67628_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542
Preparing report for the candidate 67628_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542
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Considering the candidate 67675_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542
Preparing report for the candidate 67675_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542
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Considering the candidate 67713_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542
The candidate 67713_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542 did not pass the final checks
**** FOUND 14:06:05.27 -31:41:07.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67736_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542
The candidate 67736_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542 did not pass the final checks
**** FOUND 14:08:55.25 -30:06:01.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67776_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542
The candidate 67776_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542 did not pass the final checks
**** FOUND 14:33:57.26 -31:40:43.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67806_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542
The candidate 67806_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542 did not pass the final checks
**** FOUND 14:09:28.55 -34:52:10.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67833_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542
The candidate 67833_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542 did not pass the final checks
**** FOUND 14:25:46.36 -31:30:56.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67839_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542
The candidate 67839_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542 did not pass the final checks
**** FOUND 14:49:11.87 -34:00:50.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67854_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542
The candidate 67854_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542 did not pass the final checks
**** FOUND 14:37:18.20 -30:10:52.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67866_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542
The candidate 67866_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542 did not pass the final checks
**** FOUND 14:16:59.52 -31:42:44.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67873_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542
The candidate 67873_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542 did not pass the final checks
**** FOUND 14:39:33.35 -37:08:02.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67888_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542
The candidate 67888_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542 did not pass the final checks
**** FOUND 14:08:14.89 -31:38:29.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67900_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542
The candidate 67900_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542 did not pass the final checks
**** FOUND 14:08:42.44 -30:22:48.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67901_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542
The candidate 67901_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542 did not pass the final checks
**** FOUND 14:20:20.94 -30:51:00.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67903_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542
The candidate 67903_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542 did not pass the final checks
**** FOUND 14:11:19.35 -31:11:01.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 3.866 6124714043742648704 212.83185708508 -31.18406673408 14.2085 13.6545 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.866#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67905_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542
The candidate 67905_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542 did not pass the final checks
**** FOUND 14:09:14.42 -30:34:18.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67916_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542
The candidate 67916_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542 did not pass the final checks
**** FOUND 14:07:13.74 -32:18:20.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67924_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542
The candidate 67924_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542 did not pass the final checks
**** FOUND 14:12:56.26 -31:10:27.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 1.281 6124728577911962112 213.23459920731 -31.17473635507 13.4748 12.6557 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.281#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67926_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542
The candidate 67926_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542 did not pass the final checks
**** FOUND 14:10:00.37 -31:45:47.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 0.947 6124308289592401664 212.50167373968 -31.76340448816 13.7868 13.1294 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.947#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67935_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542
The candidate 67935_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542 did not pass the final checks
**** FOUND 14:09:41.25 -30:16:40.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 1.414 6172867121121565952 212.42204393764 -30.27817036600 13.7472 13.2122 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.414#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67936_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542
The candidate 67936_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542 did not pass the final checks
**** FOUND 14:16:02.19 -32:25:20.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67939_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542
The candidate 67939_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542 did not pass the final checks
**** FOUND 14:08:40.00 -30:29:05.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67941_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542
The candidate 67941_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542 did not pass the final checks
**** FOUND 14:08:08.96 -30:44:03.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 1.631 6172830150042744320 212.03778794084 -30.73450726591 13.9497 13.4160 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.631#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67945_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542
The candidate 67945_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542 did not pass the final checks
**** FOUND 14:06:30.81 -33:01:19.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 0.999 6124079419375146112 211.62818779452 -33.02171552122 13.8358 13.3167 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.999#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 67975_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542
The candidate 67975_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542 did not pass the final checks
**** FOUND 14:27:16.64 -32:13:11.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 1.473 6219512630619486080 216.81950190267 -32.22018895887 13.7912 13.2212 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.473#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 48327_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542
The candidate 48327_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542 did not pass the final checks
**** FOUND 14:46:33.37 -31:27:20.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 41386_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542
The candidate 41386_fd_Cen-03-Q2b1x1_2026-04-19_01-24-59_20.00sec_-5.00C_LIGHT_0542 did not pass the final checks