This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461149.8171,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260419.3171 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461149.8171,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260419.3171 13.79CV 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: 2461093.94661763 22.02.2026 10:42:57.763 /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
First image: 2461093.94661763 22.02.2026 10:42:57.763 /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
Last image: 2461149.81735067 19.04.2026 07:36:49.098 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.63
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 4909
Objects passed selection criteria: 4905
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 4591.25
Average stars matched: 4487 (97.7294 %)
Memory usage VmPeak: 111244 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Apr 19 03:37:01 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: 2461093.94661763 22.02.2026 10:42:57.763 /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
First image: 2461093.94661763 22.02.2026 10:42:57.763 /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
Last image: 2461149.81735067 19.04.2026 07:36:49.098 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 68
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.33
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: 13 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): 27835
Objects passed selection criteria: 27771
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 26139.8
Average stars matched: 25006 (95.6627 %)
Memory usage VmPeak: 131064 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Apr 19 03:37:56 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-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits
SExtractor catalog cache: saved Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits.cat to cache
SExtractor catalog cache: saved Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.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-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461149.81679766
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-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits exists and is non-empty
Saving wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits to local_wcs_cache/
'wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits' -> 'local_wcs_cache/wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits'
wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits exists and is non-empty
Saving wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits to local_wcs_cache/
'wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits' -> 'local_wcs_cache/wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits'
wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits exists and is non-empty
Saving wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits to local_wcs_cache/
'wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits' -> 'local_wcs_cache/wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits'
wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits exists and is non-empty
Saving wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits to local_wcs_cache/
'wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits' -> 'local_wcs_cache/wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits (1st reference image)
verification OK: wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
Image size: 937.7'x624.9' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 13:42:51.358 +05:59:16.47 J2000 4789.000 3195.000
###################################
The image scale is 5.88"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits (1st new image)
verification OK: wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits
Image size: 937.2'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 13:42:56.870 +05:58:15.45 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 13:42:51.358 +05:59:16.47
Second-epoch image center 13:42:56.870 +05:58:15.45
Angular distance between the image centers 0.0284 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits (2nd new image)
verification OK: wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits
Image size: 937.3'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 13:42:58.915 +05:58:13.03 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 13:42:51.358 +05:59:16.47
Second-epoch image center 13:42:58.915 +05:58:13.03
Angular distance between the image centers 0.0359 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 13:42:56.870 +05:58:15.45
Second-epoch second image center 13:42:58.915 +05:58:13.03
Angular distance between the image centers 0.00850 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-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits &> /tmp/tmp.yrsk8HoQtW
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits &> /tmp/tmp.AOSLEeuPS8
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits &> /tmp/tmp.wgll2o0nOt
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits &> /tmp/tmp.cYFsiCH012
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.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-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits and wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.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-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits and wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits.cat
Found non-empty wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits and wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits.cat
The reference image (wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits) and catalog (wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits.cat) found
'wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits.cat' -> 'wcsmag.cat'
Read 6371 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 197.6203 to 214.0565 deg, Dec +0.1313 to +11.7245 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 197.6203 to 214.0565 deg, Dec 0.1313 to 11.7245 deg
Loaded 4511 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): 3361 out of 3468 total matches.
Matched with Tycho-2 3468 out of 6371 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.948201
a=0.000000 b=1.000000 c=22.948201
From vast_summary.log: estimated ref. image limiting mag.: -7.63
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.32
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.32
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.3 pix Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
2.3 pix Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
2.3 pix fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits
2.3 pix fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits
Limiting magnitude estimates:
15.3 mag. Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
15.3 mag. Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
15.1 mag. fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits
15.2 mag. fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 12.2 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.yrsk8HoQtW (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.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-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits' -> 'wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
WCS_IMAGE_NAME=wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
WCS-calibrated image found: wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
Checking if the catalog wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits.cat corresponding to the image wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits alredy exist and is non-empty...
Catalog wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits.cat corresponding to the image wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
WCS catalog name: wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=356, passed=6371
Got 6371 stars (including 6012 good ones) from the SExtractor catalog wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits.cat
util/solve_plate_with_UCAC5 got 6371 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010419 (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 450 to 510 (Dec 0.1 to 11.7)
Done reading UCAC5 zone files...
Matched 982 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 982 matched stars entering correct_measured_positions(), 976 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 982 matched stars entering correct_measured_positions(), 6292 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
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 450 to 510 (Dec 0.1 to 11.7)
Done reading UCAC5 zone files...
Matched 982 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 982 matched stars entering correct_measured_positions(), 6291 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 982 matched stars entering correct_measured_positions(), 6291 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 982 stars left (next iteration limit 1080)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits -region wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.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.AOSLEeuPS8 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.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-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits' -> 'wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
WCS_IMAGE_NAME=wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
WCS-calibrated image found: wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
Checking if the catalog wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits.cat corresponding to the image wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits alredy exist and is non-empty...
Catalog wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits.cat corresponding to the image wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
WCS catalog name: wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=378, passed=6255
Got 6255 stars (including 5875 good ones) from the SExtractor catalog wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits.cat
util/solve_plate_with_UCAC5 got 6255 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010419 (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 450 to 510 (Dec 0.1 to 11.7)
Done reading UCAC5 zone files...
Matched 982 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 982 matched stars entering correct_measured_positions(), 975 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 982 matched stars entering correct_measured_positions(), 6164 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
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 450 to 510 (Dec 0.1 to 11.7)
Done reading UCAC5 zone files...
Matched 982 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 982 matched stars entering correct_measured_positions(), 6166 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 982 matched stars entering correct_measured_positions(), 6166 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 982 stars left (next iteration limit 1080)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits -region wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.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.wgll2o0nOt (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits
WCS_IMAGE_NAME=wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits
WCS-calibrated image found: wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits
Checking if the catalog wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits.cat corresponding to the image wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits.cat corresponding to the image wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits
WCS catalog name: wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=308, passed=5542
Got 5542 stars (including 5229 good ones) from the SExtractor catalog wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits.cat
util/solve_plate_with_UCAC5 got 5542 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (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 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 967 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 5454 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
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 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 5455 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 5455 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits -region wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.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.cYFsiCH012 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits
WCS_IMAGE_NAME=wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits
WCS-calibrated image found: wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits
Checking if the catalog wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits.cat corresponding to the image wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits.cat corresponding to the image wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits
WCS catalog name: wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=328, passed=5508
Got 5508 stars (including 5179 good ones) from the SExtractor catalog wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits.cat
util/solve_plate_with_UCAC5 got 5508 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 973 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 5400 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
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 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 5400 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 5400 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits -region wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.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-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits'
Saving fully-calibrated image wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits'
Saving fully-calibrated image wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits'
Saving fully-calibrated image wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits'
Preparing the HTML report for the field Vir-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20361_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600
The candidate 20361_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600 did not pass the final checks
**** FOUND 13:47:51.84 +07:00:46.7 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-04-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-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits
SExtractor catalog cache: saved Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits.cat to cache
SExtractor catalog cache: saved Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.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-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
Creating symlink local_wcs_cache/wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.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-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits exists and is non-empty
wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits exists and is non-empty
wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits exists and is non-empty
wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits (1st reference image)
verification OK: wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
Image size: 937.7'x624.9' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 13:42:51.358 +05:59:16.47 J2000 4789.000 3195.000
###################################
The image scale is 5.88"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits (1st new image)
verification OK: wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits
Image size: 937.2'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 13:42:56.870 +05:58:15.45 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 13:42:51.358 +05:59:16.47
Second-epoch image center 13:42:56.870 +05:58:15.45
Angular distance between the image centers 0.0284 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits (2nd new image)
verification OK: wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits
Image size: 937.3'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 13:42:58.915 +05:58:13.03 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 13:42:51.358 +05:59:16.47
Second-epoch image center 13:42:58.915 +05:58:13.03
Angular distance between the image centers 0.0359 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 13:42:56.870 +05:58:15.45
Second-epoch second image center 13:42:58.915 +05:58:13.03
Angular distance between the image centers 0.00850 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-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits &> /tmp/tmp.WnDAQ4DEbl
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits &> /tmp/tmp.7ZdtgMvgm8
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits &> /tmp/tmp.J6XogWWHid
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits &> /tmp/tmp.F3JAxtNdbf
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.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-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits and wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.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-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits and wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits.cat
Found non-empty wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits and wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits.cat
The reference image (wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits) and catalog (wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits.cat) found
'wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits.cat' -> 'wcsmag.cat'
Read 33426 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 197.5473 to 214.0698 deg, Dec +0.1166 to +11.7520 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 197.5473 to 214.0698 deg, Dec 0.1166 to 11.7520 deg
Loaded 4535 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): 3241 out of 3477 total matches.
Matched with Tycho-2 3477 out of 33426 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.827622
a=0.000000 b=1.000000 c=22.827622
From vast_summary.log: estimated ref. image limiting mag.: -7.33
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.50
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.50
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 29 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
2.2 pix Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
2.2 pix fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits
2.2 pix fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits
Limiting magnitude estimates:
15.5 mag. Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
15.5 mag. Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
15.3 mag. fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits
15.3 mag. fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits
All-image limiting magnitude estimate: 15.3 (SNR ) 14.7 (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.WnDAQ4DEbl (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.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-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits' -> 'wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
WCS_IMAGE_NAME=wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
WCS-calibrated image found: wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
Checking if the catalog wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits.cat corresponding to the image wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits alredy exist and is non-empty...
Catalog wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits.cat corresponding to the image wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
WCS catalog name: wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=1360, passed=33416
Got 33416 stars (including 32008 good ones) from the SExtractor catalog wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits.cat
util/solve_plate_with_UCAC5 got 33416 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010419 (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 450 to 510 (Dec 0.1 to 11.8)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 970 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 33035 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
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 450 to 510 (Dec 0.1 to 11.8)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 33036 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 33036 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 979 stars left (next iteration limit 1076)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits -region wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.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.7ZdtgMvgm8 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.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-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits' -> 'wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
WCS_IMAGE_NAME=wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
WCS-calibrated image found: wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
Checking if the catalog wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits.cat corresponding to the image wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits alredy exist and is non-empty...
Catalog wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits.cat corresponding to the image wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
WCS catalog name: wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=1371, passed=33591
Got 33591 stars (including 32174 good ones) from the SExtractor catalog wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits.cat
util/solve_plate_with_UCAC5 got 33591 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010419 (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 450 to 510 (Dec 0.1 to 11.8)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 969 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 33126 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
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 450 to 510 (Dec 0.1 to 11.8)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 33125 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 33125 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 978 stars left (next iteration limit 1075)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits -region wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.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.J6XogWWHid (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits
WCS_IMAGE_NAME=wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits
WCS-calibrated image found: wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits
Checking if the catalog wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits.cat corresponding to the image wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits.cat corresponding to the image wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits
WCS catalog name: wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=1346, passed=29621
Got 29621 stars (including 28231 good ones) from the SExtractor catalog wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits.cat
util/solve_plate_with_UCAC5 got 29621 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (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 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 967 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 29162 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
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 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 29161 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 29161 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits -region wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.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.F3JAxtNdbf (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits
WCS_IMAGE_NAME=wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits
WCS-calibrated image found: wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits
Checking if the catalog wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits.cat corresponding to the image wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits.cat corresponding to the image wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits
WCS catalog name: wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=1348, passed=29979
Got 29979 stars (including 28585 good ones) from the SExtractor catalog wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits.cat
util/solve_plate_with_UCAC5 got 29979 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 973 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 29365 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
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 453 to 508 (Dec 0.6 to 11.3)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 29363 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 29363 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits -region wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.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-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/wcs_Vir-04-Q2b1x1_2026-02-22_04-42-57_20.00sec_-14.90C_LIGHT_0444.fits
Saving fully-calibrated image wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/wcs_Vir-04-Q2b1x1_2026-02-22_04-43-43_20.00sec_-15.00C_LIGHT_0445.fits
Saving fully-calibrated image wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-01_20.00sec_-4.90C_LIGHT_0599.fits
Saving fully-calibrated image wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_Vir-04-Q2b1x1_023735_TTUQ2b1x1_2406708_4aCQXA76/wcs_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600.fits
Preparing the HTML report for the field Vir-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out52052.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52054.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52055.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52059.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52060.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52827.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53113.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53160.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53205.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53210.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53222.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53235.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53242.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53261.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53329.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53364.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out52292.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52616.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 52052_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600
The candidate 52052_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600 did not pass the final checks
**** FOUND 13:52:37.18 +09:23:37.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.87, MAG_FAINT_SEARCH_LIMIT=15.85)GAIADR2_OUTPUT=# 1.876 3722218086930817920 208.15516099156 +09.39337136642 15.1590 14.6710 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.876#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52054_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600
The candidate 52054_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600 did not pass the final checks
**** FOUND 13:40:21.03 +02:18:49.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.57, MAG_FAINT_SEARCH_LIMIT=15.55)
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Considering the candidate 52055_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600
The candidate 52055_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600 did not pass the final checks
**** FOUND 13:35:59.70 +05:35:04.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.52, MAG_FAINT_SEARCH_LIMIT=15.50)GAIADR2_OUTPUT=# 0.735 3714875857518148224 203.99881243745 +05.58444450398 14.4426 13.6546 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.735#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52059_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600
The candidate 52059_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600 did not pass the final checks
**** FOUND 13:38:12.68 +10:12:31.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)GAIADR2_OUTPUT=# 1.287 3726072115704310400 204.55247116258 +10.20863819684 14.1019 13.4204 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.287#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52060_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600
The candidate 52060_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600 did not pass the final checks
**** FOUND 13:46:42.57 +08:45:07.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)GAIADR2_OUTPUT=# 1.820 3725067436954383232 206.67691609182 +08.75183249387 14.2815 13.4695 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.820#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52065_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600
The candidate 52065_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600 did not pass the final checks
**** FOUND 14:00:09.46 +03:55:55.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52238_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600
The candidate 52238_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600 did not pass the final checks
**** FOUND 13:55:36.53 +03:28:27.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52292_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600
Preparing report for the candidate 52292_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600
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Considering the candidate 52392_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600
The candidate 52392_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600 did not pass the final checks
**** FOUND 14:07:52.05 +02:46:20.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52565_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600
The candidate 52565_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600 did not pass the final checks
**** FOUND 14:00:28.41 +07:02:25.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52596_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600
The candidate 52596_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600 did not pass the final checks
**** FOUND 14:04:19.47 +02:35:18.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52616_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600
Preparing report for the candidate 52616_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600
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Considering the candidate 52827_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600
The candidate 52827_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600 did not pass the final checks
**** FOUND 13:49:00.61 +03:23:03.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.31, MAG_FAINT_SEARCH_LIMIT=15.29)GAIADR2_OUTPUT=# 2.319 3665674567600916096 207.25189663616 +03.38432433287 14.4731 14.0422 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.319#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52978_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600
The candidate 52978_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600 did not pass the final checks
**** FOUND 13:44:16.28 +06:02:48.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53113_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600
The candidate 53113_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600 did not pass the final checks
**** FOUND 14:08:31.85 +03:47:14.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.95, MAG_FAINT_SEARCH_LIMIT=15.93)GAIADR2_OUTPUT=# 1.102 3671015376613426688 212.13241260998 +03.78727996291 14.8304 14.3746 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.102#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53126_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600
The candidate 53126_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600 did not pass the final checks
**** FOUND 14:10:03.63 +03:49:52.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53142_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600
The candidate 53142_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600 did not pass the final checks
**** FOUND 14:06:24.50 +03:08:19.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53160_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600
The candidate 53160_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600 did not pass the final checks
**** FOUND 14:04:32.71 +02:04:10.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.93, MAG_FAINT_SEARCH_LIMIT=15.91)GAIADR2_OUTPUT=# 1.521 3661402002854437632 211.13599995708 +02.06913855361 14.8495 14.2651 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.521#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53199_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600
The candidate 53199_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600 did not pass the final checks
**** FOUND 13:53:56.70 +01:58:59.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53205_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600
The candidate 53205_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600 did not pass the final checks
**** FOUND 14:01:27.40 +05:42:29.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.87, MAG_FAINT_SEARCH_LIMIT=15.85)GAIADR2_OUTPUT=# 4.013 3672418284731003520 210.36332491189 +05.70756989270 15.3417 14.7631 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.013#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53210_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600
The candidate 53210_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600 did not pass the final checks
**** FOUND 13:52:04.02 +01:47:19.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.91, MAG_FAINT_SEARCH_LIMIT=15.89)GAIADR2_OUTPUT=# 2.000 3664183114437697280 208.01644458262 +01.78828582556 14.8961 14.3603 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.000#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53222_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600
The candidate 53222_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600 did not pass the final checks
**** FOUND 14:02:01.73 +02:39:27.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.99, MAG_FAINT_SEARCH_LIMIT=15.97)GAIADR2_OUTPUT=# 1.898 3664498949152824832 210.50668098664 +02.65772930975 14.8286 14.1939 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.898#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53235_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600
The candidate 53235_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600 did not pass the final checks
**** FOUND 14:05:09.90 +02:27:18.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.99, MAG_FAINT_SEARCH_LIMIT=15.97)GAIADR2_OUTPUT=# 1.487 3667434748278044928 211.29160152765 +02.45483788781 14.6656 13.6707 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.487#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53242_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600
The candidate 53242_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600 did not pass the final checks
**** FOUND 14:03:59.61 +02:07:19.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.91, MAG_FAINT_SEARCH_LIMIT=15.89)GAIADR2_OUTPUT=# 1.510 3661406435260690304 210.99799837377 +02.12195358936 14.9509 14.4152 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.510#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53261_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600
The candidate 53261_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600 did not pass the final checks
**** FOUND 14:09:14.54 +02:52:26.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.91, MAG_FAINT_SEARCH_LIMIT=15.89)GAIADR2_OUTPUT=# 0.271 3667511542293353984 212.31054806031 +02.87406665365 14.7795 13.9819 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.271#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53274_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600
The candidate 53274_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600 did not pass the final checks
**** FOUND 13:44:09.62 +05:22:46.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53329_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600
The candidate 53329_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600 did not pass the final checks
**** FOUND 13:43:57.09 +08:02:07.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.95, MAG_FAINT_SEARCH_LIMIT=15.93)GAIADR2_OUTPUT=# 1.656 3724626154834488832 205.98767228076 +08.03585841976 15.3537 14.8409 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.656#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53364_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600
The candidate 53364_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600 did not pass the final checks
**** FOUND 13:31:34.73 +07:59:36.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.93, MAG_FAINT_SEARCH_LIMIT=15.91)GAIADR2_OUTPUT=# 0.890 3719479169106369152 202.89495672458 +07.99349723419 14.9308 14.4025 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.890#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 09606_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600
The candidate 09606_fd_Vir-04-Q2b1x1_2026-04-19_02-36-49_20.00sec_-4.90C_LIGHT_0600 did not pass the final checks