This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 05 25.2398 2461185.7398 11.30 14:34:34.29 -18:59:30.2
334.17896 37.54402 galactic Lib Second-epoch detections are separated by 0.6" and 10.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.135 Hertha 3 -1 3 11.5 0 -0
Forced photometry on wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits at 14:34:34.29 -18:59:30.2: 15.04 +/- 99.00 upperlimit
Forced photometry on wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits at 14:34:34.29 -18:59:30.2: 15.05 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
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,2461185.7398,11.30,0.05,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 20260525.2398 11.30CV 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
Mean magnitude and position on the discovery images:
2026 05 25.2398 2461185.7398 14.02 14:30:00.30 -13:57:18.9
336.19536 42.46159 galactic Lib Second-epoch detections are separated by 0.5" and 10.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1590 Tsiolkovskaja 3 -0 3 14.0 -0 -0
Forced photometry on wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits at 14:30:00.30 -13:57:18.9: 15.33 +/- 99.00 upperlimit
Forced photometry on wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits at 14:30:00.30 -13:57:18.9: 15.30 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
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,2461185.7398,14.02,0.05,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 20260525.2398 14.02CV 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: 2461147.88334142 17.04.2026 09:11:50.699 /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
First image: 2461147.88334142 17.04.2026 09:11:50.699 /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
Last image: 2461185.74013192 25.05.2026 05:45:37.398 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.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.: -7.86
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): 3859
Objects passed selection criteria: 3856
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 3419.75
Average stars matched: 3330.25 (97.3828 %)
Memory usage VmPeak: 110460 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun May 24 19:55:43 CDT 2026
VaST build number 1.0rc89-81-g313b1a97
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-24)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon May 25 00:52:21 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: 2461147.88334142 17.04.2026 09:11:50.699 /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
First image: 2461147.88334142 17.04.2026 09:11:50.699 /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
Last image: 2461185.74013192 25.05.2026 05:45:37.398 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 31
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.54
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: 12 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): 28719
Objects passed selection criteria: 28658
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 26345.2
Average stars matched: 25481.5 (96.7214 %)
Memory usage VmPeak: 133528 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun May 24 19:55:43 CDT 2026
VaST build number 1.0rc89-81-g313b1a97
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-05-24)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon May 25 00:54:33 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-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits
SExtractor catalog cache: saved Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits.cat to cache
SExtractor catalog cache: saved Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.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-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.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: 2461185.73950565
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-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits exists and is non-empty
Saving wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits to local_wcs_cache/
'wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits' -> 'local_wcs_cache/wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits'
wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits exists and is non-empty
Saving wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits to local_wcs_cache/
'wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits' -> 'local_wcs_cache/wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits'
wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits exists and is non-empty
Saving wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits to local_wcs_cache/
'wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits' -> 'local_wcs_cache/wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits'
wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits exists and is non-empty
Saving wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits to local_wcs_cache/
'wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits' -> 'local_wcs_cache/wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits (1st reference image)
verification OK: wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
Image size: 941.4'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 14:13:21.696 -17:58:59.47 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits (1st new image)
verification OK: wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits
Image size: 937.2'x624.3' 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: 14:13:19.794 -17:59:48.78 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 14:13:21.696 -17:58:59.47
Second-epoch image center 14:13:19.794 -17:59:48.78
Angular distance between the image centers 0.0156 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits (2nd new image)
verification OK: wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.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: 14:13:23.261 -17:59:10.25 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 14:13:21.696 -17:58:59.47
Second-epoch image center 14:13:23.261 -17:59:10.25
Angular distance between the image centers 0.0069 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 14:13:19.794 -17:59:48.78
Second-epoch second image center 14:13:23.261 -17:59:10.25
Angular distance between the image centers 0.01742 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-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits &> /tmp/tmp.Xwl1yGEpKP
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits &> /tmp/tmp.ceqv3HyJaX
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits &> /tmp/tmp.7PweCOy39T
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits &> /tmp/tmp.c07lDK2JjY
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.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-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits and wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits.cat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
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-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits and wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits.cat
Found non-empty wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits and wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits.cat
The reference image (wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits) and catalog (wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits.cat) found
'wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits.cat' -> 'wcsmag.cat'
Read 5014 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 204.5767 to 221.7333 deg, Dec -23.5612 to -12.1148 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 204.5767 to 221.7333 deg, Dec -23.5612 to -12.1148 deg
Loaded 5916 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): 3786 out of 3842 total matches.
Matched with Tycho-2 3842 out of 5014 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.424350
a=0.000000 b=1.000000 c=22.424350
From vast_summary.log: estimated ref. image limiting mag.: -7.86
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.56
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.56
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 5014 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 204.5767 to 221.7333 deg, Dec -23.5612 to -12.1148 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 204.5767 to 221.7333 deg, Dec -23.5612 to -12.1148 deg
Loaded 5916 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): 3786 out of 3842 total matches.
Matched with Tycho-2 3842 out of 5014 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits:
Forced-photometry filter: calibrated wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits -> calib.txt_param_ref_wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits (aperture=6.1)
Read 4998 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 204.5768 to 221.7332 deg, Dec -23.5612 to -12.1147 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 204.5768 to 221.7332 deg, Dec -23.5612 to -12.1147 deg
Loaded 5916 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): 3802 out of 3860 total matches.
Matched with Tycho-2 3860 out of 4998 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits:
Forced-photometry filter: calibrated wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits -> calib.txt_param_ref_wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits (aperture=6.1)
____ 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:
2.2 pix Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
2.2 pix Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
2.2 pix fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits
2.2 pix fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits
2.2 pix wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
2.2 pix wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
Limiting magnitude estimates:
14.6 mag. Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
14.6 mag. Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
14.2 mag. fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits
14.2 mag. fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 11.2 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.Xwl1yGEpKP (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.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-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits' -> 'wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
WCS_IMAGE_NAME=wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
WCS-calibrated image found: wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
Checking if the catalog wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits.cat corresponding to the image wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits alredy exist and is non-empty...
Catalog wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits.cat corresponding to the image wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
WCS catalog name: wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=275, passed=5014
Got 5014 stars (including 4733 good ones) from the SExtractor catalog wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits.cat
util/solve_plate_with_UCAC5 got 5014 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 332 to 391 (Dec -23.6 to -12.1)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 960 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 4960 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 332 to 391 (Dec -23.6 to -12.1)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 4961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 4961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits N_match=968 sigma_overall_arcsec=0.350 sigma_q1_arcsec=0.407 sigma_q2_arcsec=0.429 sigma_q3_arcsec=0.309 sigma_q4_arcsec=0.286 n_q1=235 n_q2=224 n_q3=274 n_q4=235 worst_quadrant_to_overall_ratio=1.225
The image catalog is written to wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits -region wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.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.ceqv3HyJaX (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.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-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits' -> 'wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
WCS_IMAGE_NAME=wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
WCS-calibrated image found: wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
Checking if the catalog wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits.cat corresponding to the image wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits alredy exist and is non-empty...
Catalog wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits.cat corresponding to the image wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
WCS catalog name: wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=275, passed=4998
Got 4998 stars (including 4713 good ones) from the SExtractor catalog wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits.cat
util/solve_plate_with_UCAC5 got 4998 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 332 to 391 (Dec -23.6 to -12.1)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 4947 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 332 to 391 (Dec -23.6 to -12.1)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 4948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 4948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits N_match=969 sigma_overall_arcsec=0.356 sigma_q1_arcsec=0.377 sigma_q2_arcsec=0.423 sigma_q3_arcsec=0.336 sigma_q4_arcsec=0.299 n_q1=234 n_q2=224 n_q3=277 n_q4=234 worst_quadrant_to_overall_ratio=1.188
The image catalog is written to wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits -region wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.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.7PweCOy39T (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_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.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_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits
WCS_IMAGE_NAME=wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits
WCS-calibrated image found: wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits
Checking if the catalog wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits.cat corresponding to the image wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits.cat corresponding to the image wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits
WCS catalog name: wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=269, passed=3669
Got 3669 stars (including 3392 good ones) from the SExtractor catalog wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits.cat
util/solve_plate_with_UCAC5 got 3669 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 333 to 388 (Dec -23.2 to -12.7)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 959 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 3624 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 388 (Dec -23.2 to -12.7)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 3623 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 3623 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits N_match=968 sigma_overall_arcsec=0.491 sigma_q1_arcsec=0.427 sigma_q2_arcsec=0.533 sigma_q3_arcsec=0.445 sigma_q4_arcsec=0.530 n_q1=224 n_q2=248 n_q3=262 n_q4=234 worst_quadrant_to_overall_ratio=1.085
The image catalog is written to wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits -region wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.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.c07lDK2JjY (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_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.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_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits
WCS_IMAGE_NAME=wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits
WCS-calibrated image found: wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits
Checking if the catalog wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits.cat corresponding to the image wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits.cat corresponding to the image wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits
WCS catalog name: wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=265, passed=3695
Got 3695 stars (including 3429 good ones) from the SExtractor catalog wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits.cat
util/solve_plate_with_UCAC5 got 3695 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 333 to 388 (Dec -23.2 to -12.7)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 962 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 3658 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 388 (Dec -23.2 to -12.7)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 3660 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 3660 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits N_match=968 sigma_overall_arcsec=0.464 sigma_q1_arcsec=0.358 sigma_q2_arcsec=0.588 sigma_q3_arcsec=0.411 sigma_q4_arcsec=0.528 n_q1=214 n_q2=252 n_q3=261 n_q4=241 worst_quadrant_to_overall_ratio=1.268
The image catalog is written to wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits -region wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits sigma_overall=0.350 worst_q_ratio=1.225
ref2=Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits sigma_overall=0.356 worst_q_ratio=1.188
new1=fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits sigma_overall=0.491 worst_q_ratio=1.085
new2=fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits sigma_overall=0.464 worst_q_ratio=1.268
reference average sigma_overall=0.353 worst_q_ratio=1.2065
warn-on-ratio threshold: 2.0x reference
###################################
Distribution of catalog-matched stars across the image:
plot_astrometric_residuals_xy: wrote wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261_astrometric_residuals.png (968 matched stars from wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262_astrometric_residuals.png (969 matched stars from wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186_astrometric_residuals.png (968 matched stars from wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits.cat.astrometric_residuals, image 9576x6388)
plot_astrometric_residuals_xy: wrote wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187_astrometric_residuals.png (968 matched stars from wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits.cat.astrometric_residuals, image 9576x6388)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits'
Saving fully-calibrated image wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits'
Preparing the HTML report for the field Vir-14-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits at 14:34:34.29 -18:59:30.2: 15.04 +/- 99.00 upperlimit
Forced photometry on wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits at 14:34:34.29 -18:59:30.2: 15.05 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out20318.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 20318_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187
Preparing report for the candidate 20318_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 8s
Prepared the HTML report for the field Vir-14-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
14:34:34.29 -18:59:30.2
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits
SExtractor catalog cache: saved Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits.cat to cache
SExtractor catalog cache: saved Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.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-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
Creating symlink local_wcs_cache/wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.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-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits exists and is non-empty
wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits exists and is non-empty
wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits exists and is non-empty
wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits (1st reference image)
verification OK: wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
Image size: 941.4'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 14:13:21.696 -17:58:59.47 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits (1st new image)
verification OK: wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits
Image size: 937.2'x624.3' 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: 14:13:19.794 -17:59:48.78 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 14:13:21.696 -17:58:59.47
Second-epoch image center 14:13:19.794 -17:59:48.78
Angular distance between the image centers 0.0156 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits (2nd new image)
verification OK: wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.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: 14:13:23.261 -17:59:10.25 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 14:13:21.696 -17:58:59.47
Second-epoch image center 14:13:23.261 -17:59:10.25
Angular distance between the image centers 0.0069 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 14:13:19.794 -17:59:48.78
Second-epoch second image center 14:13:23.261 -17:59:10.25
Angular distance between the image centers 0.01742 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-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits &> /tmp/tmp.BKiNKT90zG
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits &> /tmp/tmp.7WIcW6caLe
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits &> /tmp/tmp.nlFEn1c3pI
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits &> /tmp/tmp.x2KoHzQ8zP
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.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-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits and wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits.cat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
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-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits and wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits.cat
Found non-empty wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits and wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits.cat
The reference image (wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits) and catalog (wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits.cat) found
'wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits.cat' -> 'wcsmag.cat'
Read 36862 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 204.4759 to 221.7592 deg, Dec -23.5830 to -12.0587 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 204.4759 to 221.7592 deg, Dec -23.5830 to -12.0587 deg
Loaded 5989 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): 4525 out of 4790 total matches.
Matched with Tycho-2 4790 out of 36862 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.270300
a=0.000000 b=1.000000 c=22.270300
From vast_summary.log: estimated ref. image limiting mag.: -7.54
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.73
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.73
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 36862 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 204.4759 to 221.7592 deg, Dec -23.5830 to -12.0587 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 204.4759 to 221.7592 deg, Dec -23.5830 to -12.0587 deg
Loaded 5989 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): 4525 out of 4790 total matches.
Matched with Tycho-2 4790 out of 36862 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits:
Forced-photometry filter: calibrated wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits -> calib.txt_param_ref_wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits (aperture=4.6)
Read 36742 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 204.4745 to 221.7495 deg, Dec -23.6101 to -12.0717 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 204.4745 to 221.7495 deg, Dec -23.6101 to -12.0717 deg
Loaded 5994 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): 4524 out of 4787 total matches.
Matched with Tycho-2 4787 out of 36742 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits:
Forced-photometry filter: calibrated wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits -> calib.txt_param_ref_wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits (aperture=4.6)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 22 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
2.0 pix Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
2.0 pix fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits
2.0 pix fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits
2.0 pix wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
2.0 pix wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
Limiting magnitude estimates:
14.7 mag. Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
14.7 mag. Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
14.3 mag. fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits
14.3 mag. fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 13.8 (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.BKiNKT90zG (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.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-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits' -> 'wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
WCS_IMAGE_NAME=wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
WCS-calibrated image found: wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
Checking if the catalog wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits.cat corresponding to the image wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits alredy exist and is non-empty...
Catalog wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits.cat corresponding to the image wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits
WCS catalog name: wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=1188, passed=36842
Got 36842 stars (including 35599 good ones) from the SExtractor catalog wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits.cat
util/solve_plate_with_UCAC5 got 36842 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 332 to 391 (Dec -23.6 to -12.1)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 36562 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 332 to 391 (Dec -23.6 to -12.1)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 36564 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 36564 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits N_match=971 sigma_overall_arcsec=0.332 sigma_q1_arcsec=0.381 sigma_q2_arcsec=0.395 sigma_q3_arcsec=0.298 sigma_q4_arcsec=0.294 n_q1=234 n_q2=224 n_q3=274 n_q4=239 worst_quadrant_to_overall_ratio=1.192
The image catalog is written to wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits -region wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.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.7WIcW6caLe (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.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-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits' -> 'wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
WCS_IMAGE_NAME=wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
WCS-calibrated image found: wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
Checking if the catalog wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits.cat corresponding to the image wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits alredy exist and is non-empty...
Catalog wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits.cat corresponding to the image wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits
WCS catalog name: wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=1195, passed=36729
Got 36729 stars (including 35480 good ones) from the SExtractor catalog wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits.cat
util/solve_plate_with_UCAC5 got 36729 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 331 to 391 (Dec -23.6 to -12.1)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 36416 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
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 331 to 391 (Dec -23.6 to -12.1)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 36417 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 36417 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits N_match=970 sigma_overall_arcsec=0.339 sigma_q1_arcsec=0.380 sigma_q2_arcsec=0.370 sigma_q3_arcsec=0.313 sigma_q4_arcsec=0.299 n_q1=235 n_q2=221 n_q3=273 n_q4=241 worst_quadrant_to_overall_ratio=1.118
The image catalog is written to wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits -region wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.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.nlFEn1c3pI (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_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.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_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits
WCS_IMAGE_NAME=wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits
WCS-calibrated image found: wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits
Checking if the catalog wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits.cat corresponding to the image wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits.cat corresponding to the image wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits
WCS catalog name: wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=864, passed=26375
Got 26375 stars (including 25471 good ones) from the SExtractor catalog wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits.cat
util/solve_plate_with_UCAC5 got 26375 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 333 to 388 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 26054 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 388 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 26054 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 969 matched stars entering correct_measured_positions(), 26054 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits N_match=969 sigma_overall_arcsec=0.494 sigma_q1_arcsec=0.420 sigma_q2_arcsec=0.542 sigma_q3_arcsec=0.475 sigma_q4_arcsec=0.535 n_q1=227 n_q2=245 n_q3=275 n_q4=222 worst_quadrant_to_overall_ratio=1.096
The image catalog is written to wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits -region wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.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.x2KoHzQ8zP (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_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.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_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits
WCS_IMAGE_NAME=wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits
WCS-calibrated image found: wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits
Checking if the catalog wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits.cat corresponding to the image wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits.cat corresponding to the image wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits
WCS catalog name: wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=856, passed=26397
Got 26397 stars (including 25505 good ones) from the SExtractor catalog wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits.cat
util/solve_plate_with_UCAC5 got 26397 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 333 to 388 (Dec -23.2 to -12.6)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 26064 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 388 (Dec -23.2 to -12.6)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 26063 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 26063 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits N_match=970 sigma_overall_arcsec=0.464 sigma_q1_arcsec=0.344 sigma_q2_arcsec=0.605 sigma_q3_arcsec=0.434 sigma_q4_arcsec=0.490 n_q1=222 n_q2=242 n_q3=277 n_q4=229 worst_quadrant_to_overall_ratio=1.302
The image catalog is written to wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits -region wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.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_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-44-43_20.00sec_5.00C_LIGHT_0186.fits
Saving fully-calibrated image wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.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_2026-05-25_CI_Vir-14-Q2b1x1_005006_TTUQ2b1x1_1390303_EbRjm7AP/wcs_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187.fits
Preparing the HTML report for the field Vir-14-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits at 14:41:50.75 -20:02:11.8: 13.81 +/- 0.11 detection
Forced photometry on wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits at 14:33:32.41 -15:00:14.2: 13.03 +/- 0.05 detection
Forced photometry on wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits at 14:36:40.30 -21:11:52.5: 12.92 +/- 0.05 detection
Forced photometry on wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits at 14:18:47.79 -18:37:15.4: 14.10 +/- 0.13 detection
Forced photometry on wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits at 14:19:16.65 -15:14:46.8: 13.59 +/- 0.08 detection
Forced photometry on wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits at 14:29:08.05 -18:54:35.5: 13.07 +/- 0.05 detection
Forced photometry on wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits at 14:40:56.02 -18:47:05.3: 13.14 +/- 0.06 detection
Forced photometry on wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits at 13:59:04.49 -21:30:48.8: 13.57 +/- 0.08 detection
Forced photometry on wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits at 14:41:50.75 -20:02:11.8: 13.76 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.79 +/- 0.08
Forced photometry filter REJECTED candidate at 14:41:50.75 -20:02:11.8: ref_mag=13.79 +/- 0.08 new_mean_mag=13.7789 delta=0.01 (need > 0.90)
Forced photometry on wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits at 14:33:32.41 -15:00:14.2: 13.10 +/- 0.06 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.04
Forced photometry filter REJECTED candidate at 14:33:32.41 -15:00:14.2: ref_mag=13.07 +/- 0.04 new_mean_mag=13.2191 delta=-0.15 (need > 0.90)
Forced photometry on wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits at 14:19:16.65 -15:14:46.8: 13.58 +/- 0.08 detection
Forced photometry on wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits at 14:36:40.30 -21:11:52.5: 12.87 +/- 0.05 detection
Forced photometry on wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits at 14:18:47.79 -18:37:15.4: 14.11 +/- 0.13 detection
Forced photometry reference-image weighted average: 13.58 +/- 0.05
Forced photometry reference-image weighted average: 12.89 +/- 0.04
Forced photometry filter REJECTED candidate at 14:19:16.65 -15:14:46.8: ref_mag=13.58 +/- 0.05 new_mean_mag=13.6920 delta=-0.11 (need > 0.90)
Forced photometry reference-image weighted average: 14.11 +/- 0.09
Forced photometry filter REJECTED candidate at 14:36:40.30 -21:11:52.5: ref_mag=12.89 +/- 0.04 new_mean_mag=12.8804 delta=0.01 (need > 0.90)
Forced photometry filter REJECTED candidate at 14:18:47.79 -18:37:15.4: ref_mag=14.11 +/- 0.09 new_mean_mag=14.1139 delta=-0.01 (need > 0.90)
Forced photometry on wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits at 13:59:04.49 -21:30:48.8: 13.56 +/- 0.08 detection
Forced photometry on wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits at 14:40:56.02 -18:47:05.3: 13.12 +/- 0.06 detection
Forced photometry on wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits at 14:29:08.05 -18:54:35.5: 13.11 +/- 0.05 detection
Forced photometry reference-image weighted average: 13.56 +/- 0.06
Forced photometry filter REJECTED candidate at 13:59:04.49 -21:30:48.8: ref_mag=13.56 +/- 0.06 new_mean_mag=13.7154 delta=-0.15 (need > 0.90)
Forced photometry reference-image weighted average: 13.13 +/- 0.04
Forced photometry filter REJECTED candidate at 14:40:56.02 -18:47:05.3: ref_mag=13.13 +/- 0.04 new_mean_mag=13.2816 delta=-0.15 (need > 0.90)
Forced photometry reference-image weighted average: 13.09 +/- 0.04
Forced photometry filter REJECTED candidate at 14:29:08.05 -18:54:35.5: ref_mag=13.09 +/- 0.04 new_mean_mag=13.2086 delta=-0.12 (need > 0.90)
Forced photometry on wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits at 14:41:19.91 -17:27:27.9: 14.05 +/- 0.13 detection
Forced photometry on wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits at 14:37:48.11 -19:46:31.5: 14.57 +/- 0.21 detection
Forced photometry on wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits at 14:30:00.30 -13:57:18.9: 15.33 +/- 99.00 upperlimit
Forced photometry on wcs_Vir-14-Q2b1x1_2026-04-17_04-11-50_20.00sec_-4.90C_LIGHTs_0261.fits at 14:29:25.88 -18:14:51.7: 13.91 +/- 0.11 detection
Forced photometry on wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits at 14:37:48.11 -19:46:31.5: 14.39 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.47 +/- 0.14
Forced photometry on wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits at 14:41:19.91 -17:27:27.9: 14.12 +/- 0.14 detection
Forced photometry filter REJECTED candidate at 14:37:48.11 -19:46:31.5: ref_mag=14.47 +/- 0.14 new_mean_mag=13.9518 delta=0.52 (need > 0.90)
Forced photometry reference-image weighted average: 14.09 +/- 0.09
Forced photometry filter REJECTED candidate at 14:41:19.91 -17:27:27.9: ref_mag=14.09 +/- 0.09 new_mean_mag=13.8544 delta=0.23 (need > 0.90)
Forced photometry on wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits at 14:30:00.30 -13:57:18.9: 15.30 +/- 99.00 upperlimit
Forced photometry on wcs_Vir-14-Q2b1x1_2026-04-17_04-12-48_20.00sec_-5.00C_LIGHTs_0262.fits at 14:29:25.88 -18:14:51.7: 14.20 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.02 +/- 0.09
Forced photometry filter REJECTED candidate at 14:29:25.88 -18:14:51.7: ref_mag=14.02 +/- 0.09 new_mean_mag=14.0271 delta=-0.01 (need > 0.90)
Adding exclusion_list_local.txt__out53139.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 52536_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187
The candidate 52536_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187 did not pass the final checks
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Considering the candidate 52538_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187
The candidate 52538_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187 did not pass the final checks
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Considering the candidate 52543_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187
The candidate 52543_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187 did not pass the final checks
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Considering the candidate 52629_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187
The candidate 52629_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187 did not pass the final checks
**** FOUND 14:34:34.28 -18:59:30.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52778_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187
The candidate 52778_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187 did not pass the final checks
**** FOUND 14:31:28.98 -17:00:54.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52785_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187
The candidate 52785_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187 did not pass the final checks
**** FOUND 14:29:34.21 -15:01:33.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52795_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187
The candidate 52795_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187 did not pass the final checks
**** FOUND 14:06:37.70 -14:10:42.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52845_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187
The candidate 52845_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187 did not pass the final checks
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Considering the candidate 52869_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187
The candidate 52869_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187 did not pass the final checks
**** FOUND 14:37:28.97 -20:19:41.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52886_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187
The candidate 52886_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187 did not pass the final checks
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Considering the candidate 52899_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187
The candidate 52899_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187 did not pass the final checks
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Considering the candidate 52904_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187
The candidate 52904_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187 did not pass the final checks
**** FOUND 14:15:19.34 -18:13:07.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 52945_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187
The candidate 52945_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187 did not pass the final checks
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Considering the candidate 52986_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187
The candidate 52986_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187 did not pass the final checks
**** FOUND 14:06:34.71 -17:26:00.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53018_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187
The candidate 53018_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187 did not pass the final checks
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Considering the candidate 53029_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187
The candidate 53029_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187 did not pass the final checks
**** FOUND 14:08:03.71 -19:44:12.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53047_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187
The candidate 53047_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187 did not pass the final checks
**** FOUND 14:22:31.26 -15:45:11.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53081_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187
The candidate 53081_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187 did not pass the final checks
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Considering the candidate 53093_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187
The candidate 53093_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187 did not pass the final checks
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Considering the candidate 53139_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187
Preparing report for the candidate 53139_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187
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Considering the candidate 53166_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187
The candidate 53166_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187 did not pass the final checks
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Considering the candidate 15582_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187
The candidate 15582_fd_Vir-14-Q2b1x1_2026-05-25_00-45-37_20.00sec_5.00C_LIGHT_0187 did not pass the final checks