This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 19.2503* 13 19 13.43 -21 05 05.5 12.5 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461149.7503,12.53,0.05,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 20260419.2503 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 19.2503* 13 08 06.11 -20 39 07.7 13.5 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461149.7503,13.46,0.05,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 20260419.2503 13.46CV 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: 2461098.91064843 27.02.2026 09:51:10.024 /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
First image: 2461098.91064843 27.02.2026 09:51:10.024 /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
Last image: 2461149.75061094 19.04.2026 06:00:42.785 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
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: 5 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): 4754
Objects passed selection criteria: 4740
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 3684.25
Average stars matched: 3374.75 (91.5994 %)
Memory usage VmPeak: 110492 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 01:03:29 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.91064843 27.02.2026 09:51:10.024 /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
First image: 2461098.91064843 27.02.2026 09:51:10.024 /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
Last image: 2461149.75061094 19.04.2026 06:00:42.785 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 40
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.85
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: 15 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): 29655
Objects passed selection criteria: 29585
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 23758.5
Average stars matched: 21824.5 (91.8598 %)
Memory usage VmPeak: 130560 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 01:04:36 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/Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits
SExtractor catalog cache: saved Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat to cache
SExtractor catalog cache: saved Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.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/Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.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: 2461149.74997017
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_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits exists and is non-empty
Saving wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits to local_wcs_cache/
'wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits' -> 'local_wcs_cache/wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits'
wcs_Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits exists and is non-empty
Saving wcs_Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits to local_wcs_cache/
'wcs_Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits' -> 'local_wcs_cache/wcs_Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits'
wcs_fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits exists and is non-empty
Saving wcs_fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits to local_wcs_cache/
'wcs_fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits' -> 'local_wcs_cache/wcs_fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits'
wcs_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits exists and is non-empty
Saving wcs_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits to local_wcs_cache/
'wcs_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits' -> 'local_wcs_cache/wcs_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits (1st reference image)
verification OK: wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
Image size: 941.6'x627.3' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 13:20:00.735 -18:00:04.53 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits (1st new image)
verification OK: wcs_fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits
Image size: 937.6'x624.6' 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: 13:20:04.882 -17:57:13.68 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 13:20:00.735 -18:00:04.53
Second-epoch image center 13:20:04.882 -17:57:13.68
Angular distance between the image centers 0.0502 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits (2nd new image)
verification OK: wcs_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits
Image size: 937.6'x624.6' 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: 13:20:02.520 -17:57:10.16 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 13:20:00.735 -18:00:04.53
Second-epoch image center 13:20:02.520 -17:57:10.16
Angular distance between the image centers 0.0490 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 13:20:04.882 -17:57:13.68
Second-epoch second image center 13:20:02.520 -17:57:10.16
Angular distance between the image centers 0.00941 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/Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits &> /tmp/tmp.PTASB9wzSC
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits &> /tmp/tmp.ISV4fUN86z
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits &> /tmp/tmp.j4oqdqPQau
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits &> /tmp/tmp.nxd747oFpP
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.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_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits and wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.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_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits and wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat
Found non-empty wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits and wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat
The reference image (wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits) and catalog (wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat) found
'wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat' -> 'wcsmag.cat'
Read 5029 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 191.6471 to 208.5697 deg, Dec -23.3251 to -12.4821 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 191.6471 to 208.5697 deg, Dec -23.3251 to -12.4821 deg
Loaded 5144 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): 3620 out of 3751 total matches.
Matched with Tycho-2 3751 out of 5029 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.817526
a=0.000000 b=1.000000 c=22.817526
From vast_summary.log: estimated ref. image limiting mag.: -8.17
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.65
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.65
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
2.1 pix Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
2.7 pix fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits
2.7 pix fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits
Limiting magnitude estimates:
14.7 mag. Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
14.6 mag. Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
14.3 mag. fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits
14.3 mag. fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 11.6 (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.PTASB9wzSC (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits is already a symlink and we do not allow symlinks on symlinks
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_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits' -> 'wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
WCS_IMAGE_NAME=wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
WCS-calibrated image found: wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
Checking if the catalog wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat corresponding to the image wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits alredy exist and is non-empty...
Catalog wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat corresponding to the image wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
WCS catalog name: wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=403, passed=5029
Got 5029 stars (including 4621 good ones) from the SExtractor catalog wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat
util/solve_plate_with_UCAC5 got 5029 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 4965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 4964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 4964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits -region wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.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.ISV4fUN86z (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits is already a symlink and we do not allow symlinks on symlinks
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_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits' -> 'wcs_Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
WCS_IMAGE_NAME=wcs_Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
WCS-calibrated image found: wcs_Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
Checking if the catalog wcs_Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits.cat corresponding to the image wcs_Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits alredy exist and is non-empty...
Catalog wcs_Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits.cat corresponding to the image wcs_Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
WCS catalog name: wcs_Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=395, passed=5063
Got 5063 stars (including 4663 good ones) from the SExtractor catalog wcs_Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits.cat
util/solve_plate_with_UCAC5 got 5063 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 5002 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 5002 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 5002 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits -region wcs_Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.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.j4oqdqPQau (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_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.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_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits
WCS_IMAGE_NAME=wcs_fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits
WCS-calibrated image found: wcs_fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits
Checking if the catalog wcs_fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits.cat corresponding to the image wcs_fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits.cat corresponding to the image wcs_fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.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_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits
WCS catalog name: wcs_fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=365, passed=4641
Got 4641 stars (including 4272 good ones) from the SExtractor catalog wcs_fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits.cat
util/solve_plate_with_UCAC5 got 4641 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 333 to 389 (Dec -23.2 to -12.5)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 4597 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
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 333 to 389 (Dec -23.2 to -12.5)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 4598 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 4598 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits -region wcs_fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.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.nxd747oFpP (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_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.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_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits
WCS_IMAGE_NAME=wcs_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits
WCS-calibrated image found: wcs_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits
Checking if the catalog wcs_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits.cat corresponding to the image wcs_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits.cat corresponding to the image wcs_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.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_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits
WCS catalog name: wcs_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=369, passed=4606
Got 4606 stars (including 4231 good ones) from the SExtractor catalog wcs_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits.cat
util/solve_plate_with_UCAC5 got 4606 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 333 to 389 (Dec -23.2 to -12.5)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 970 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 4563 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
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 333 to 389 (Dec -23.2 to -12.5)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 4563 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 4563 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits -region wcs_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.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_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits'
Saving fully-calibrated image wcs_Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/wcs_Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits'
Saving fully-calibrated image wcs_fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/wcs_fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits'
Saving fully-calibrated image wcs_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/wcs_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits'
Preparing the HTML report for the field Vir-13-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out21011.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20870_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524
The candidate 20870_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524 did not pass the final checks
**** FOUND 13:16:01.83 -17:14:50.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20872_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524
The candidate 20872_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524 did not pass the final checks
**** FOUND 13:19:46.10 -20:37:45.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20946_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524
The candidate 20946_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524 did not pass the final checks
**** FOUND 13:32:13.32 -19:39:50.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21011_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524
The candidate 21011_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524 did not pass the final checks
**** FOUND 13:20:14.96 -19:05:17.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.74, MAG_FAINT_SEARCH_LIMIT=12.72)GAIADR2_OUTPUT=# 0.259 3507777168774849280 200.06230763420 -19.08804348834 11.5892 11.1037 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.259#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Vir-13-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/Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits
SExtractor catalog cache: saved Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat to cache
SExtractor catalog cache: saved Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
Creating symlink local_wcs_cache/wcs_Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.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_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits exists and is non-empty
wcs_Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits exists and is non-empty
wcs_fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits exists and is non-empty
wcs_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits (1st reference image)
verification OK: wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
Image size: 941.6'x627.3' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 13:20:00.735 -18:00:04.53 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits (1st new image)
verification OK: wcs_fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits
Image size: 937.6'x624.6' 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: 13:20:04.882 -17:57:13.68 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 13:20:00.735 -18:00:04.53
Second-epoch image center 13:20:04.882 -17:57:13.68
Angular distance between the image centers 0.0502 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits (2nd new image)
verification OK: wcs_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits
Image size: 937.6'x624.6' 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: 13:20:02.520 -17:57:10.16 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 13:20:00.735 -18:00:04.53
Second-epoch image center 13:20:02.520 -17:57:10.16
Angular distance between the image centers 0.0490 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 13:20:04.882 -17:57:13.68
Second-epoch second image center 13:20:02.520 -17:57:10.16
Angular distance between the image centers 0.00941 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/Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits &> /tmp/tmp.AuJJtJTqE0
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits &> /tmp/tmp.R4l2EGFIZz
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits &> /tmp/tmp.FL2LonVCsq
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits &> /tmp/tmp.R5G2TRyUJR
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.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_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits and wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.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_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits and wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat
Found non-empty wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits and wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat
The reference image (wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits) and catalog (wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat) found
'wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat' -> 'wcsmag.cat'
Read 33033 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 191.6273 to 208.6562 deg, Dec -23.3283 to -12.4172 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 191.6273 to 208.6562 deg, Dec -23.3283 to -12.4172 deg
Loaded 5201 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): 4068 out of 4378 total matches.
Matched with Tycho-2 4378 out of 33033 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.639476
a=0.000000 b=1.000000 c=22.639476
From vast_summary.log: estimated ref. image limiting mag.: -7.85
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.79
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.79
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 21 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
2.1 pix Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
2.4 pix fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits
2.3 pix fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits
Limiting magnitude estimates:
14.8 mag. Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
14.8 mag. Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
14.5 mag. fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits
14.5 mag. fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 14.0 (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.AuJJtJTqE0 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits is already a symlink and we do not allow symlinks on symlinks
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_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits' -> 'wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
WCS_IMAGE_NAME=wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
WCS-calibrated image found: wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
Checking if the catalog wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat corresponding to the image wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits alredy exist and is non-empty...
Catalog wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat corresponding to the image wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
WCS catalog name: wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=1226, passed=33026
Got 33026 stars (including 31740 good ones) from the SExtractor catalog wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat
util/solve_plate_with_UCAC5 got 33026 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.4)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 966 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 32624 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
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 333 to 389 (Dec -23.3 to -12.4)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 32622 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 32622 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits -region wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.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.R4l2EGFIZz (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits is already a symlink and we do not allow symlinks on symlinks
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_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits' -> 'wcs_Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
WCS_IMAGE_NAME=wcs_Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
WCS-calibrated image found: wcs_Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
Checking if the catalog wcs_Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits.cat corresponding to the image wcs_Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits alredy exist and is non-empty...
Catalog wcs_Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits.cat corresponding to the image wcs_Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
WCS catalog name: wcs_Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=1202, passed=32717
Got 32717 stars (including 31458 good ones) from the SExtractor catalog wcs_Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits.cat
util/solve_plate_with_UCAC5 got 32717 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.4)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 967 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 32341 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
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 333 to 389 (Dec -23.3 to -12.4)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 32342 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 32342 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits -region wcs_Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.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.FL2LonVCsq (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_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.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_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits
WCS_IMAGE_NAME=wcs_fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits
WCS-calibrated image found: wcs_fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits
Checking if the catalog wcs_fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits.cat corresponding to the image wcs_fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits.cat corresponding to the image wcs_fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.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_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits
WCS catalog name: wcs_fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=21, blended=1160, passed=28229
Got 28229 stars (including 27032 good ones) from the SExtractor catalog wcs_fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits.cat
util/solve_plate_with_UCAC5 got 28229 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 333 to 389 (Dec -23.2 to -12.5)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 27965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
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 333 to 389 (Dec -23.2 to -12.5)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 27965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 27965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits -region wcs_fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.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.R5G2TRyUJR (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_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.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_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits
WCS_IMAGE_NAME=wcs_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits
WCS-calibrated image found: wcs_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits
Checking if the catalog wcs_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits.cat corresponding to the image wcs_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits.cat corresponding to the image wcs_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.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_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits
WCS catalog name: wcs_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=25, blended=1151, passed=28496
Got 28496 stars (including 27307 good ones) from the SExtractor catalog wcs_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits.cat
util/solve_plate_with_UCAC5 got 28496 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 333 to 389 (Dec -23.2 to -12.5)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 28232 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.2 to -12.5)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 28233 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 28233 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits -region wcs_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.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_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.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_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/wcs_Vir-13-Q2b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
Saving fully-calibrated image wcs_Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.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_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/wcs_Vir-13-Q2b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
Saving fully-calibrated image wcs_fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.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_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/wcs_fd_Vir-13-Q2b1x1_2026-04-19_00-59-47_20.00sec_-4.90C_LIGHT_0523.fits
Saving fully-calibrated image wcs_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.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_Vir-13-Q2b1x1_010120_TTUQ2b1x1_2490675_7HWBrxbl/wcs_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524.fits
Preparing the HTML report for the field Vir-13-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out51980.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56001.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56255.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56328.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56380.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56407.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56430.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56464.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56472.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56475.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out56438.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out53352.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55103.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: 2s
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Considering the candidate 51980_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524
The candidate 51980_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524 did not pass the final checks
**** FOUND 13:31:15.38 -16:42:04.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 1.226 3603829031403593984 202.81385380462 -16.70148227643 13.1187 12.6000 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.226#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51983_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524
The candidate 51983_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524 did not pass the final checks
**** FOUND 13:06:25.70 -14:04:59.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53352_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524
Preparing report for the candidate 53352_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54805_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524
The candidate 54805_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524 did not pass the final checks
**** FOUND 13:32:24.88 -20:09:37.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55103_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524
Preparing report for the candidate 55103_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56001_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524
The candidate 56001_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524 did not pass the final checks
**** FOUND 13:21:26.38 -21:20:06.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.19, MAG_FAINT_SEARCH_LIMIT=15.17)GAIADR2_OUTPUT=# 0.496 3506193395289518208 200.35977848845 -21.33521553385 14.4317 13.8517 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.496#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56026_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524
The candidate 56026_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524 did not pass the final checks
**** FOUND 13:36:58.83 -19:49:15.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56125_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524
The candidate 56125_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524 did not pass the final checks
**** FOUND 13:37:33.93 -20:50:08.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56211_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524
The candidate 56211_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524 did not pass the final checks
**** FOUND 13:34:18.69 -20:55:25.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56224_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524
The candidate 56224_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524 did not pass the final checks
**** FOUND 13:23:27.23 -21:46:31.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56255_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524
The candidate 56255_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524 did not pass the final checks
**** FOUND 13:34:20.70 -19:37:36.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.42, MAG_FAINT_SEARCH_LIMIT=15.40)GAIADR2_OUTPUT=# 0.817 6292974850760696448 203.58604854315 -19.62665342933 14.5663 14.0221 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.817#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56328_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524
The candidate 56328_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524 did not pass the final checks
**** FOUND 13:36:32.40 -21:29:52.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.32, MAG_FAINT_SEARCH_LIMIT=15.30)GAIADR2_OUTPUT=# 0.879 6195728029446050944 204.13515581481 -21.49760917075 14.3549 13.6496 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.879#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56380_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524
The candidate 56380_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524 did not pass the final checks
**** FOUND 13:35:42.99 -17:02:38.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)GAIADR2_OUTPUT=# 1.426 3603582019244580352 203.92916279284 -17.04442214845 14.3847 13.7572 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.426#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56407_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524
The candidate 56407_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524 did not pass the final checks
**** FOUND 13:10:48.06 -22:00:19.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.31, MAG_FAINT_SEARCH_LIMIT=15.29)GAIADR2_OUTPUT=# 1.725 3504703144717166976 197.70052120326 -22.00503642997 14.3038 13.7617 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.725#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56430_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524
The candidate 56430_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524 did not pass the final checks
**** FOUND 13:25:21.84 -22:03:32.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 1.295 6196058467049884288 201.34106517270 -22.05870096067 14.4338 13.8346 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.295#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56438_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524
The candidate 56438_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524 did not pass the final checks
**** FOUND 13:24:41.40 -20:12:14.8 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)
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Considering the candidate 56464_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524
The candidate 56464_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524 did not pass the final checks
**** FOUND 13:18:29.57 -21:05:60.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.32, MAG_FAINT_SEARCH_LIMIT=15.30)GAIADR2_OUTPUT=# 2.494 3506177899047503744 199.62310799541 -21.09931358612 14.3455 13.5687 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.494#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56472_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524
The candidate 56472_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524 did not pass the final checks
**** FOUND 13:19:06.72 -21:36:56.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)GAIADR2_OUTPUT=# 0.727 3506080901506042624 199.77821510114 -21.61566663394 14.2106 13.5193 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.727#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56475_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524
The candidate 56475_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524 did not pass the final checks
**** FOUND 13:10:23.89 -21:12:24.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.30, MAG_FAINT_SEARCH_LIMIT=15.28)GAIADR2_OUTPUT=# 2.830 3505633778230735744 197.60014076371 -21.20622470492 14.3744 13.8782 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.830#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56585_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524
The candidate 56585_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524 did not pass the final checks
**** FOUND 13:19:07.43 -19:08:28.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32176_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524
The candidate 32176_fd_Vir-13-Q2b1x1_2026-04-19_01-00-42_20.00sec_-5.00C_LIGHT_0524 did not pass the final checks