This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL
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 09.2627* 13 27 33.04 -22 03 25.0 12.7 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,2461139.7627,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260409.2627 12.66CV 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 09.2627* 13 16 42.66 -21 50 22.5 13.7 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,2461139.7627,13.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260409.2627 13.70CV 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: 2461139.76302881 09.04.2026 06:18:35.689 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.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: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 5474
Objects passed selection criteria: 5451
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: 4180
Average stars matched: 3666 (87.7033 %)
Memory usage VmPeak: 111008 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 9 01:36:33 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: 2461139.76302881 09.04.2026 06:18:35.689 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 39
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: 10 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): 31951
Objects passed selection criteria: 31878
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: 25180.8
Average stars matched: 22712.8 (90.1989 %)
Memory usage VmPeak: 131224 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 9 01:37:15 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_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.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_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461139.76237043
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_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits exists and is non-empty
Saving wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits to local_wcs_cache/
'wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits' -> 'local_wcs_cache/wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits'
wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits exists and is non-empty
Saving wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits to local_wcs_cache/
'wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits' -> 'local_wcs_cache/wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 13:20:00.735 -18:00:04.53
Second-epoch image center 13:19:57.946 -17:58:34.63
Angular distance between the image centers 0.0273 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 13:20:00.735 -18:00:04.53
Second-epoch image center 13:19:54.978 -17:58:15.10
Angular distance between the image centers 0.0380 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 13:19:57.946 -17:58:34.63
Second-epoch second image center 13:19:54.978 -17:58:15.10
Angular distance between the image centers 0.01295 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.WdMl0CAYNh
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.MuCyi0tcNA
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_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits &> /tmp/tmp.CfDg2vQvbt
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits &> /tmp/tmp.SJIwGQyzJY
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.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: 3000)
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
3.1 pix fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits
3.1 pix fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.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
14.5 mag. fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits
14.5 mag. fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 11.7 (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.WdMl0CAYNh (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_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/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.MuCyi0tcNA (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_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/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.CfDg2vQvbt (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits
WCS_IMAGE_NAME=wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits
WCS-calibrated image found: wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits
Checking if the catalog wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits.cat corresponding to the image wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits.cat corresponding to the image wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.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_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits
WCS catalog name: wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=487, passed=5680
Got 5680 stars (including 5191 good ones) from the SExtractor catalog wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits.cat
util/solve_plate_with_UCAC5 got 5680 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (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(), 957 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 5580 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
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(), 5580 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 5580 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
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_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits -region wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.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.SJIwGQyzJY (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits
WCS_IMAGE_NAME=wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits
WCS-calibrated image found: wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits
Checking if the catalog wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits.cat corresponding to the image wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits.cat corresponding to the image wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.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_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits
WCS catalog name: wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=517, passed=5720
Got 5720 stars (including 5198 good ones) from the SExtractor catalog wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits.cat
util/solve_plate_with_UCAC5 got 5720 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (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 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 958 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 5568 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
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 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 5569 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 5569 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits -region wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.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_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/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_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/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_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits'
Saving fully-calibrated image wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits'
Preparing the HTML report for the field Vir-13-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20964_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223
The candidate 20964_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223 did not pass the final checks
**** FOUND 13:32:13.22 -19:39:50.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20983_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223
The candidate 20983_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223 did not pass the final checks
**** FOUND 13:16:01.86 -17:14:50.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21022_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223
The candidate 21022_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223 did not pass the final checks
**** FOUND 13:13:55.05 -14:28:30.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21035_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223
The candidate 21035_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223 did not pass the final checks
**** FOUND 13:19:46.13 -20:37:45.4 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field 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_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.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_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.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_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.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_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits exists and is non-empty
wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 13:20:00.735 -18:00:04.53
Second-epoch image center 13:19:57.946 -17:58:34.63
Angular distance between the image centers 0.0273 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 13:20:00.735 -18:00:04.53
Second-epoch image center 13:19:54.978 -17:58:15.10
Angular distance between the image centers 0.0380 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 13:19:57.946 -17:58:34.63
Second-epoch second image center 13:19:54.978 -17:58:15.10
Angular distance between the image centers 0.01295 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.67o6tmSKXX
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.zMf1onD8Uv
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_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits &> /tmp/tmp.6dORNwVirZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits &> /tmp/tmp.5IybFzvcMS
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.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 26 candidate transients before the final filtering. (Hard limit: 3000)
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
2.7 pix fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits
2.6 pix fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.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
14.7 mag. fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits
14.7 mag. fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 14.1 (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.67o6tmSKXX (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_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/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.zMf1onD8Uv (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_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/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.6dORNwVirZ (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits
WCS_IMAGE_NAME=wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits
WCS-calibrated image found: wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits
Checking if the catalog wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits.cat corresponding to the image wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits.cat corresponding to the image wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.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_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits
WCS catalog name: wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=2445, passed=28403
Got 28403 stars (including 25929 good ones) from the SExtractor catalog wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits.cat
util/solve_plate_with_UCAC5 got 28403 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (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 -23.3 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(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 27583 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 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(), 27584 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 27584 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
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_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits -region wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.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.5IybFzvcMS (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits
WCS_IMAGE_NAME=wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits
WCS-calibrated image found: wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits
Checking if the catalog wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits.cat corresponding to the image wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits.cat corresponding to the image wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.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_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits
WCS catalog name: wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=2423, passed=28765
Got 28765 stars (including 26312 good ones) from the SExtractor catalog wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits.cat
util/solve_plate_with_UCAC5 got 28765 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (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 -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 960 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 28094 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
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 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 28095 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 28095 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits -region wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.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_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/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_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/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_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-17-38_20.00sec_-5.00C_LIGHT_0222.fits
Saving fully-calibrated image wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Vir-13-Q2b1x1_013335_TTUQ2b1x1_21505_mP4bxfwL/wcs_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223.fits
Preparing the HTML report for the field Vir-13-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out51976.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51978.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51981.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57183.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57204.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57242.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57255.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57321.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57335.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57578.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57632.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57726.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57835.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out54221.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55897.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 51976_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223
The candidate 51976_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223 did not pass the final checks
**** FOUND 13:38:31.96 -18:58:20.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.09, MAG_FAINT_SEARCH_LIMIT=15.07)GAIADR2_OUTPUT=# 4.062 6292933997031899008 204.63202066764 -18.97270255366 13.7025 13.1690 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.062#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51978_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223
The candidate 51978_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223 did not pass the final checks
**** FOUND 13:04:47.29 -19:17:08.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 2.075 3509120089084322432 196.19718443823 -19.28505059138 13.9871 12.8738 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.075#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51981_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223
The candidate 51981_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223 did not pass the final checks
**** FOUND 13:18:36.36 -14:35:37.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 1.121 3607944400347268864 199.65164206144 -14.59408506333 14.0883 13.5841 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.121#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51983_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223
The candidate 51983_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223 did not pass the final checks
**** FOUND 13:06:25.85 -14:05:03.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54221_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223
Preparing report for the candidate 54221_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223
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Considering the candidate 54952_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223
The candidate 54952_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223 did not pass the final checks
**** FOUND 13:12:03.73 -16:10:13.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 55587_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223
The candidate 55587_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223 did not pass the final checks
**** FOUND 13:24:25.24 -14:06:21.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55897_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223
Preparing report for the candidate 55897_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223
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Considering the candidate 56181_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223
The candidate 56181_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223 did not pass the final checks
**** FOUND 13:12:41.53 -14:17:55.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56559_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223
The candidate 56559_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223 did not pass the final checks
**** FOUND 13:02:03.49 -14:52:57.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57183_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223
The candidate 57183_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223 did not pass the final checks
**** FOUND 13:11:46.78 -16:30:05.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 0.913 3511615018406672000 197.94473281814 -16.50137340356 14.2210 13.5846 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.913#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 57186_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223
The candidate 57186_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223 did not pass the final checks
**** FOUND 13:02:20.28 -15:46:00.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57204_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223
The candidate 57204_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223 did not pass the final checks
**** FOUND 13:13:59.59 -14:17:00.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)GAIADR2_OUTPUT=# 0.471 3608940386083318144 198.49842152991 -14.28356346098 14.2611 13.7190 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.471#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 57242_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223
The candidate 57242_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223 did not pass the final checks
**** FOUND 13:06:51.93 -15:35:46.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.28, MAG_FAINT_SEARCH_LIMIT=15.26)GAIADR2_OUTPUT=# 0.855 3512578671629104000 196.71629198276 -15.59633469840 14.1810 13.5170 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.855#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 57255_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223
The candidate 57255_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223 did not pass the final checks
**** FOUND 13:12:21.34 -21:17:44.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.22, MAG_FAINT_SEARCH_LIMIT=15.20)GAIADR2_OUTPUT=# 0.634 3504872778745258752 198.08900062076 -21.29559227936 14.5278 13.6375 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.634#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 57321_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223
The candidate 57321_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223 did not pass the final checks
**** FOUND 13:04:59.51 -13:54:56.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.48, MAG_FAINT_SEARCH_LIMIT=15.46)GAIADR2_OUTPUT=# 0.926 3620986532397959168 196.24786264464 -13.91590648882 14.3214 13.8329 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.926#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 57335_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223
The candidate 57335_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223 did not pass the final checks
**** FOUND 13:04:51.91 -17:30:20.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)GAIADR2_OUTPUT=# 0.228 3511823204061548288 196.21630500110 -17.50552119691 14.4055 13.8867 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.228#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 57433_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223
The candidate 57433_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223 did not pass the final checks
**** FOUND 13:05:25.12 -16:57:33.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57447_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223
The candidate 57447_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223 did not pass the final checks
**** FOUND 13:23:19.86 -14:53:27.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57493_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223
The candidate 57493_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223 did not pass the final checks
**** FOUND 13:10:01.30 -14:58:24.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57578_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223
The candidate 57578_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223 did not pass the final checks
**** FOUND 13:01:44.68 -19:18:22.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.35, MAG_FAINT_SEARCH_LIMIT=15.33)GAIADR2_OUTPUT=# 1.590 3509294430396754304 195.43659879214 -19.30616374143 13.5683 12.3142 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.590#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 57632_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223
The candidate 57632_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223 did not pass the final checks
**** FOUND 13:05:55.45 -19:14:44.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 1.698 3509077173771108096 196.48132238935 -19.24611244571 14.5003 13.9541 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.698#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 57652_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223
The candidate 57652_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223 did not pass the final checks
**** FOUND 13:31:03.19 -16:07:46.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57726_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223
The candidate 57726_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223 did not pass the final checks
**** FOUND 13:06:38.69 -19:40:53.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 0.630 3506042933995353600 196.66110456126 -19.68146594109 14.2116 13.5822 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.630#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 57835_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223
The candidate 57835_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223 did not pass the final checks
**** FOUND 13:04:42.83 -20:53:24.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)GAIADR2_OUTPUT=# 0.520 3505803824575859328 196.17861293907 -20.89025121467 14.3033 13.7723 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.520#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32176_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223
The candidate 32176_fd_Vir-13-Q2b1x1_2026-04-09_01-18-35_20.00sec_-5.00C_LIGHT_0223 did not pass the final checks