This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 17.3490* 13 47 37.14 -17 38 51.3 10.8 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461147.8490,10.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260417.3490 10.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 17.3490* 13 41 28.47 -13 33 09.2 12.0 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461147.8490,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260417.3490 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 17.3490* 13 20 47.24 -21 16 59.6 12.5 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461147.8490,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260417.3490 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 17.3490* 13 09 41.17 -20 53 41.9 13.4 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461147.8490,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260417.3490 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.91064843 27.02.2026 09:51:10.024 /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
First image: 2461098.91064843 27.02.2026 09:51:10.024 /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
Last image: 2461147.84940081 17.04.2026 08:22:58.230 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.18
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 5239
Objects passed selection criteria: 5233
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 4851.75
Average stars matched: 4689 (96.6455 %)
Memory usage VmPeak: 111020 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Apr 17 03:25:01 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.91064843 27.02.2026 09:51:10.024 /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
First image: 2461098.91064843 27.02.2026 09:51:10.024 /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
Last image: 2461147.84940081 17.04.2026 08:22:58.230 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 58
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.89
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): 34744
Objects passed selection criteria: 34647
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 32483.8
Average stars matched: 30863 (95.0106 %)
Memory usage VmPeak: 134992 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Apr 17 03:25:48 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/TTUQ1b1x1/TTUQ1_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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits
SExtractor catalog cache: saved Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat to cache
SExtractor catalog cache: saved Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.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: 2461147.84865833
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits exists and is non-empty
Saving wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits to local_wcs_cache/
'wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits' -> 'local_wcs_cache/wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits'
wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits exists and is non-empty
Saving wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits to local_wcs_cache/
'wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits' -> 'local_wcs_cache/wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits'
wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits exists and is non-empty
Saving wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits to local_wcs_cache/
'wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits' -> 'local_wcs_cache/wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits'
wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits exists and is non-empty
Saving wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits to local_wcs_cache/
'wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits' -> 'local_wcs_cache/wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits (1st reference image)
verification OK: wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
Image size: 941.6'x627.3' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 13:20:00.735 -18:00:04.53 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits (1st new image)
verification OK: wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits
Image size: 941.4'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 13:20:09.176 -17:58:36.59 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 13:20:00.735 -18:00:04.53
Second-epoch image center 13:20:09.176 -17:58:36.59
Angular distance between the image centers 0.0414 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits (2nd new image)
verification OK: wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits
Image size: 941.4'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 13:20:07.186 -17:58:08.05 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 13:20:00.735 -18:00:04.53
Second-epoch image center 13:20:07.186 -17:58:08.05
Angular distance between the image centers 0.0412 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 13:20:09.176 -17:58:36.59
Second-epoch second image center 13:20:07.186 -17:58:08.05
Angular distance between the image centers 0.01118 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits &> /tmp/tmp.3Hdanxujos
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits &> /tmp/tmp.hroQndJbLR
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits &> /tmp/tmp.iQZ5JcQLhS
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits &> /tmp/tmp.1slyYIXdB1
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits and wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits and wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat
Found non-empty wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits and wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat
The reference image (wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits) and catalog (wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat) found
'wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat' -> 'wcsmag.cat'
Read 5029 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 191.6471 to 208.5697 deg, Dec -23.3251 to -12.4821 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 191.6471 to 208.5697 deg, Dec -23.3251 to -12.4821 deg
Loaded 5144 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 3620 out of 3751 total matches.
Matched with Tycho-2 3751 out of 5029 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.824361
a=0.000000 b=1.000000 c=22.824361
From vast_summary.log: estimated ref. image limiting mag.: -8.18
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.64
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.64
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
2.1 pix Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
2.3 pix fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits
2.3 pix fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits
Limiting magnitude estimates:
14.6 mag. Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
14.6 mag. Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
14.6 mag. fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits
14.6 mag. fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 11.6 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.3Hdanxujos (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits' -> 'wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
WCS_IMAGE_NAME=wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
WCS-calibrated image found: wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
Checking if the catalog wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat corresponding to the image wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits alredy exist and is non-empty...
Catalog wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat corresponding to the image wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
WCS catalog name: wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=403, passed=5029
Got 5029 stars (including 4621 good ones) from the SExtractor catalog wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat
util/solve_plate_with_UCAC5 got 5029 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 4965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 4964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 4964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits -region wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.hroQndJbLR (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits' -> 'wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
WCS_IMAGE_NAME=wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
WCS-calibrated image found: wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
Checking if the catalog wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits.cat corresponding to the image wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits alredy exist and is non-empty...
Catalog wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits.cat corresponding to the image wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
WCS catalog name: wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=395, passed=5063
Got 5063 stars (including 4663 good ones) from the SExtractor catalog wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits.cat
util/solve_plate_with_UCAC5 got 5063 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 5002 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 5001 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 5001 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits -region wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.iQZ5JcQLhS (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits
WCS_IMAGE_NAME=wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits
WCS-calibrated image found: wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits
Checking if the catalog wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits.cat corresponding to the image wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits.cat corresponding to the image wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits
WCS catalog name: wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=287, passed=4785
Got 4785 stars (including 4489 good ones) from the SExtractor catalog wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits.cat
util/solve_plate_with_UCAC5 got 4785 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 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: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 4713 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
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 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(), 4713 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 4713 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits -region wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.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.1slyYIXdB1 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits
WCS_IMAGE_NAME=wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits
WCS-calibrated image found: wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits
Checking if the catalog wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits.cat corresponding to the image wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits.cat corresponding to the image wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits
WCS catalog name: wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=290, passed=4643
Got 4643 stars (including 4346 good ones) from the SExtractor catalog wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits.cat
util/solve_plate_with_UCAC5 got 4643 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 -23.5 to -12.2)
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(), 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: 970 matched stars entering correct_measured_positions(), 4574 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 332 to 391 (Dec -23.5 to -12.2)
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(), 4577 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 970 matched stars entering correct_measured_positions(), 4577 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits -region wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits'
Saving fully-calibrated image wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits'
Saving fully-calibrated image wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits'
Saving fully-calibrated image wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits'
Preparing the HTML report for the field Vir-13-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out20344.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20266_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 20266_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 12:53:58.78 -18:02:06.3 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20344_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
Preparing report for the candidate 20344_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20418_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 20418_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 13:49:24.56 -16:39:26.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20453_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 20453_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 13:32:13.33 -19:39:50.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02207_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 02207_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 13:00:41.24 -17:38:47.8 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 6s
Prepared the HTML report for the field Vir-13-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
13:47:37.14 -17:38:51.3
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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits
SExtractor catalog cache: saved Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat to cache
SExtractor catalog cache: saved Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
Creating symlink local_wcs_cache/wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits exists and is non-empty
wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits exists and is non-empty
wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits exists and is non-empty
wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits (1st reference image)
verification OK: wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
Image size: 941.6'x627.3' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 13:20:00.735 -18:00:04.53 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits (1st new image)
verification OK: wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits
Image size: 941.4'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 13:20:09.176 -17:58:36.59 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 13:20:00.735 -18:00:04.53
Second-epoch image center 13:20:09.176 -17:58:36.59
Angular distance between the image centers 0.0414 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits (2nd new image)
verification OK: wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits
Image size: 941.4'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 13:20:07.186 -17:58:08.05 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 13:20:00.735 -18:00:04.53
Second-epoch image center 13:20:07.186 -17:58:08.05
Angular distance between the image centers 0.0412 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 13:20:09.176 -17:58:36.59
Second-epoch second image center 13:20:07.186 -17:58:08.05
Angular distance between the image centers 0.01118 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits &> /tmp/tmp.0Cv0q2VWAx
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits &> /tmp/tmp.OpzbMF2Rug
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits &> /tmp/tmp.1QKJllPgx7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits &> /tmp/tmp.F2oeEAh2oU
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits and wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits and wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat
Found non-empty wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits and wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat
The reference image (wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits) and catalog (wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat) found
'wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat' -> 'wcsmag.cat'
Read 33033 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 191.6273 to 208.6562 deg, Dec -23.3283 to -12.4172 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 191.6273 to 208.6562 deg, Dec -23.3283 to -12.4172 deg
Loaded 5201 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 4068 out of 4378 total matches.
Matched with Tycho-2 4378 out of 33033 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.651881
a=0.000000 b=1.000000 c=22.651881
From vast_summary.log: estimated ref. image limiting mag.: -7.89
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.76
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.76
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 53 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
2.1 pix Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
2.0 pix fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits
2.0 pix fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits
Limiting magnitude estimates:
14.8 mag. Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
14.8 mag. Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
14.7 mag. fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits
14.7 mag. fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 14.1 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.0Cv0q2VWAx (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits' -> 'wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
WCS_IMAGE_NAME=wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
WCS-calibrated image found: wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
Checking if the catalog wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat corresponding to the image wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits alredy exist and is non-empty...
Catalog wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat corresponding to the image wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
WCS catalog name: wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=1226, passed=33024
Got 33024 stars (including 31738 good ones) from the SExtractor catalog wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat
util/solve_plate_with_UCAC5 got 33024 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.4)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 966 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 32599 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.4)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 32598 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 32598 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits -region wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.OpzbMF2Rug (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits' -> 'wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
WCS_IMAGE_NAME=wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
WCS-calibrated image found: wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
Checking if the catalog wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits.cat corresponding to the image wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits alredy exist and is non-empty...
Catalog wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits.cat corresponding to the image wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
WCS catalog name: wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=1202, passed=32716
Got 32716 stars (including 31457 good ones) from the SExtractor catalog wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits.cat
util/solve_plate_with_UCAC5 got 32716 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.4)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 966 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 32336 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.4)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 32336 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 972 matched stars entering correct_measured_positions(), 32336 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits -region wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.1QKJllPgx7 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits
WCS_IMAGE_NAME=wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits
WCS-calibrated image found: wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits
Checking if the catalog wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits.cat corresponding to the image wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits.cat corresponding to the image wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits
WCS catalog name: wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=1007, passed=32612
Got 32612 stars (including 31543 good ones) from the SExtractor catalog wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits.cat
util/solve_plate_with_UCAC5 got 32612 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 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(), 963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 32141 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 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(), 32141 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 32141 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits -region wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.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.F2oeEAh2oU (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits
WCS_IMAGE_NAME=wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits
WCS-calibrated image found: wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits
Checking if the catalog wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits.cat corresponding to the image wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits.cat corresponding to the image wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits
WCS catalog name: wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=984, passed=32507
Got 32507 stars (including 31472 good ones) from the SExtractor catalog wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits.cat
util/solve_plate_with_UCAC5 got 32507 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 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 32002 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 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(), 32003 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 32003 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits -region wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/wcs_Vir-13-Q1b1x1_2026-02-27_03-51-10_20.00sec_-14.90C_LIGHT_0478.fits
Saving fully-calibrated image wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/wcs_Vir-13-Q1b1x1_2026-02-27_03-51-50_20.00sec_-14.90C_LIGHT_0479.fits
Saving fully-calibrated image wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-21-54_20.00sec_-5.00C_LIGHTs_0225.fits
Saving fully-calibrated image wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Vir-13-Q1b1x1_032352_TTUQ1b1x1_491950_p9J1xKsC/wcs_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226.fits
Preparing the HTML report for the field Vir-13-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out53276.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53433.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53462.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53559.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53583.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53668.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53669.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53678.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53686.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53712.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53721.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53722.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53743.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53744.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53798.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53818.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out53700.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out52650.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52799.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53173.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52397_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 52397_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 13:22:42.07 -15:35:40.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52398_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 52398_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 13:24:08.30 -15:50:38.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52400_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 52400_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 12:55:10.35 -13:03:18.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52401_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 52401_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 12:55:53.25 -13:02:13.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52403_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 52403_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 13:07:24.55 -12:51:03.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52405_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 52405_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 13:06:25.80 -14:05:02.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52407_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 52407_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 12:53:58.77 -18:02:06.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52485_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 52485_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 13:47:37.14 -17:38:51.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52650_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
Preparing report for the candidate 52650_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
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Considering the candidate 52799_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
Preparing report for the candidate 52799_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
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Considering the candidate 52938_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 52938_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 12:58:48.80 -15:07:29.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53093_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 53093_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 13:12:03.69 -16:10:12.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 53096_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 53096_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 13:14:08.54 -12:45:20.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53173_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
Preparing report for the candidate 53173_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
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Considering the candidate 53186_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 53186_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 13:24:25.28 -14:06:20.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53241_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 53241_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 13:24:25.52 -15:10:02.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53276_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 53276_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 13:37:46.30 -15:57:19.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 0.370 3605437685634445568 204.44296099063 -15.95562125082 13.8187 13.1858 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.370#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53348_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 53348_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 13:51:50.01 -22:34:37.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53362_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 53362_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 13:05:50.36 -12:55:03.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53393_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 53393_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 13:12:41.44 -14:17:54.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53409_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 53409_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 13:17:58.84 -14:43:50.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53411_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 53411_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 13:32:24.77 -20:09:36.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53433_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 53433_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 13:05:30.33 -13:58:11.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 1.494 3620982306150157696 196.37679175744 -13.96989871051 14.0404 13.4783 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.494#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53462_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 53462_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 13:21:42.64 -13:58:27.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 1.288 3608366441013685120 200.42802867607 -13.97426514134 14.0559 13.2692 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.288#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53513_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 53513_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 13:32:31.97 -15:17:17.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53518_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 53518_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 13:05:05.49 -12:47:39.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53559_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 53559_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 13:51:48.21 -13:32:09.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.11, MAG_FAINT_SEARCH_LIMIT=15.09)GAIADR2_OUTPUT=# 1.183 3612016682178917888 207.95089950025 -13.53618878167 14.2387 13.7112 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.183#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53562_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 53562_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 13:33:51.35 -22:41:47.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53564_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 53564_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 13:30:24.14 -14:18:29.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53583_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 53583_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 13:13:43.51 -13:38:08.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)GAIADR2_OUTPUT=# 1.250 3609047000055555072 198.43162846656 -13.63557881239 14.4061 13.8739 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.250#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53584_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 53584_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 13:19:39.05 -18:30:40.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53630_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 53630_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 13:20:04.69 -17:07:17.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53632_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 53632_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 12:52:31.83 -14:47:48.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53640_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 53640_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 13:06:51.88 -15:35:46.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53646_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 53646_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 13:16:28.32 -22:31:56.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53668_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 53668_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 13:00:08.09 -20:02:36.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)
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Considering the candidate 53669_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 53669_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 13:48:28.34 -21:30:12.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 0.886 6288612572737433600 207.11828337977 -21.50368864127 14.2584 13.7758 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.886#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53678_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 53678_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 12:51:14.82 -15:16:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 2.220 3525210033007677056 192.81112236195 -15.26983901095 14.3197 13.8160 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.220#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53686_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 53686_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 13:29:40.83 -18:41:17.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)GAIADR2_OUTPUT=# 0.911 3602990550708331008 202.42004246937 -18.68798165647 14.5734 13.9335 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.911#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53700_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 53700_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 12:54:46.61 -13:05:14.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)
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Considering the candidate 53708_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 53708_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 12:55:40.78 -16:01:43.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53712_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 53712_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 12:52:29.31 -14:28:28.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.35, MAG_FAINT_SEARCH_LIMIT=15.33)GAIADR2_OUTPUT=# 0.613 3525417771985691136 193.12208576514 -14.47441732661 14.2325 13.7200 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.613#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53718_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 53718_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 13:13:05.36 -19:31:19.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53719_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 53719_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 12:51:19.09 -15:47:45.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53721_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 53721_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 13:50:27.95 -18:12:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 0.527 6294118377213372928 207.61659698312 -18.21034198775 14.3222 13.7928 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.527#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53722_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 53722_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 13:12:06.01 -18:41:32.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 0.531 3507699898018267392 198.02493866676 -18.69238845339 14.3669 13.7884 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.531#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53743_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 53743_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 12:50:57.81 -13:50:34.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)
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Considering the candidate 53744_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 53744_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 12:56:30.73 -15:18:56.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)GAIADR2_OUTPUT=# 0.259 3524516103731629952 194.12800506932 -15.31549298630 14.1939 13.4575 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.259#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53795_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 53795_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 12:53:12.34 -18:09:57.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53798_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 53798_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 13:39:23.58 -21:03:26.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 0.523 6291822493855364480 204.84827585949 -21.05758758085 14.3872 13.7751 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.523#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53818_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 53818_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 13:02:49.25 -19:53:20.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.32, MAG_FAINT_SEARCH_LIMIT=15.30)GAIADR2_OUTPUT=# 1.204 3508981997295840768 195.70497912182 -19.88914472752 14.1646 13.4099 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.204#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32176_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 32176_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks
**** FOUND 13:32:13.34 -19:39:50.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 14492_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226
The candidate 14492_fd_Vir-13-Q1b1x1_2026-04-17_03-22-58_20.00sec_-4.90C_LIGHTs_0226 did not pass the final checks