This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j
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 03 26.2850* 12 54 50.74 +12 56 17.5 12.1 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461125.7850,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260326.2850 12.10CV 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
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:54:50.74 +12:56:17.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20_00sec_-15_00C_LIGHT_0415_fits__*pix.png resample_wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20_00sec_-10_00C_LIGHT_0531_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20_00sec_-15_00C_LIGHT_0415_fits__*pix.png resample_wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20_00sec_-10_00C_LIGHT_0530_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20_00sec_-15_00C_LIGHT_0415_fits__*pix.png resample_wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20_00sec_-10_00C_LIGHT_0531_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20_00sec_-15_00C_LIGHT_0415_fits__*pix.png resample_wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20_00sec_-10_00C_LIGHT_0530_fits__*pix.png animation_v2.gif
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 03 26.2850* 12 55 22.39 +10 11 26.3 14.1 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461125.7850,14.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.2850 14.07CV 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
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 12:55:22.39 +10:11:26.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20_00sec_-15_00C_LIGHT_0415_fits__*pix.png resample_wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20_00sec_-10_00C_LIGHT_0531_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20_00sec_-15_00C_LIGHT_0415_fits__*pix.png resample_wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20_00sec_-10_00C_LIGHT_0530_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20_00sec_-15_00C_LIGHT_0415_fits__*pix.png resample_wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20_00sec_-10_00C_LIGHT_0531_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20_00sec_-15_00C_LIGHT_0415_fits__*pix.png resample_wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20_00sec_-10_00C_LIGHT_0530_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 26.2850 2461125.7850 14.60 13:40:23.58 +12:13:21.8
342.91031 71.18817 galactic Boo Second-epoch detections are separated by 0.4" and 7.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 3740258220884128384 | 13:40:25.90 +12:13:53.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3740258220884128384,2461125.7850,14.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3740258220884128384 20260326.2850 14.60CV 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
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 13:40:23.58 +12:13:21.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20_00sec_-15_00C_LIGHT_0415_fits__*pix.png resample_wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20_00sec_-10_00C_LIGHT_0531_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20_00sec_-15_00C_LIGHT_0415_fits__*pix.png resample_wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20_00sec_-10_00C_LIGHT_0530_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20_00sec_-15_00C_LIGHT_0415_fits__*pix.png resample_wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20_00sec_-10_00C_LIGHT_0531_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20_00sec_-15_00C_LIGHT_0415_fits__*pix.png resample_wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20_00sec_-10_00C_LIGHT_0530_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461093.92714109 22.02.2026 10:14:54.990 /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
First image: 2461093.92714109 22.02.2026 10:14:54.990 /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
Last image: 2461125.78531954 26.03.2026 06:50:41.608 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.57
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): 5431
Objects passed selection criteria: 5418
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 4467
Average stars matched: 4217.75 (94.4202 %)
Memory usage VmPeak: 111436 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 26 01:57:30 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461093.92714109 22.02.2026 10:14:54.990 /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
First image: 2461093.92714109 22.02.2026 10:14:54.990 /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
Last image: 2461125.78531954 26.03.2026 06:50:41.608 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 29
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.27
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: 8 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): 28515
Objects passed selection criteria: 28436
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 24394.2
Average stars matched: 22926 (93.9812 %)
Memory usage VmPeak: 130136 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 26 01:58:11 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits
SExtractor catalog cache: saved Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat to cache
SExtractor catalog cache: saved Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.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-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.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: 2461125.78475722
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits exists and is non-empty
Saving wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits to local_wcs_cache/
'wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits' -> 'local_wcs_cache/wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits'
wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits exists and is non-empty
Saving wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits to local_wcs_cache/
'wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits' -> 'local_wcs_cache/wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits'
wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits exists and is non-empty
Saving wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits to local_wcs_cache/
'wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits' -> 'local_wcs_cache/wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits'
wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits exists and is non-empty
Saving wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits to local_wcs_cache/
'wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits' -> 'local_wcs_cache/wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits'
The image scale is 5.88"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 13:20:00.311 +13:59:16.89
Second-epoch image center 13:19:54.309 +13:58:22.91
Angular distance between the image centers 0.03 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 13:20:00.311 +13:59:16.89
Second-epoch image center 13:19:51.569 +13:57:59.94
Angular distance between the image centers 0.04 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 13:19:54.309 +13:58:22.91
Second-epoch second image center 13:19:51.569 +13:57:59.94
Angular distance between the image centers 0.01278 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-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits &> /tmp/tmp.UQvM0tvM4O
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits &> /tmp/tmp.T8O2mbKgmK
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits &> /tmp/tmp.XEYI1Xip1Y
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits &> /tmp/tmp.qjBhWF8Qy3
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.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-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits and wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.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-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits and wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat
Found non-empty wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits and wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat
The reference image (wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits) and catalog (wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat) found
'wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat' -> 'wcsmag.cat'
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
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 3002 out of 5868 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.944237
a=0.000000 b=1.000000 c=22.944237
From vast_summary.log: estimated ref. image limiting mag.: -7.57
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.37
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.37
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
2.3 pix Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
2.4 pix fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits
2.4 pix fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits
Limiting magnitude estimates:
15.4 mag. Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
15.4 mag. Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
15.1 mag. fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits
15.1 mag. fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 12.1 (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.UQvM0tvM4O (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_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.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-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits' -> 'wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
WCS_IMAGE_NAME=wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
WCS-calibrated image found: wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
Checking if the catalog wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat corresponding to the image wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits alredy exist and is non-empty...
Catalog wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat corresponding to the image wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
WCS catalog name: wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=363, passed=5868
Got 5868 stars (including 5502 good ones) from the SExtractor catalog wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat
util/solve_plate_with_UCAC5 got 5868 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.40"
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits -region wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.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.T8O2mbKgmK (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_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.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-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits' -> 'wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
WCS_IMAGE_NAME=wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
WCS-calibrated image found: wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
Checking if the catalog wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits.cat corresponding to the image wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits alredy exist and is non-empty...
Catalog wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits.cat corresponding to the image wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
WCS catalog name: wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=372, passed=5872
Got 5872 stars (including 5497 good ones) from the SExtractor catalog wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits.cat
util/solve_plate_with_UCAC5 got 5872 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.40"
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits -region wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.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.XEYI1Xip1Y (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_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.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_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits
WCS_IMAGE_NAME=wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits
WCS-calibrated image found: wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits
Checking if the catalog wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits.cat corresponding to the image wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits.cat corresponding to the image wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits
WCS catalog name: wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=328, passed=4908
Got 4908 stars (including 4577 good ones) from the SExtractor catalog wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits.cat
util/solve_plate_with_UCAC5 got 4908 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.37"
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits -region wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.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.qjBhWF8Qy3 (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_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.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_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits
WCS_IMAGE_NAME=wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits
WCS-calibrated image found: wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits
Checking if the catalog wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits.cat corresponding to the image wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits.cat corresponding to the image wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits
WCS catalog name: wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=313, passed=4854
Got 4854 stars (including 4536 good ones) from the SExtractor catalog wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits.cat
util/solve_plate_with_UCAC5 got 4854 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
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...
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.38"
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits -region wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.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-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits'
Saving fully-calibrated image wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits'
Saving fully-calibrated image wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits'
Saving fully-calibrated image wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits'
Preparing the HTML report for the field Vir-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out20751.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 20751_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531
Preparing report for the candidate 20751_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531
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-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
12:54:50.74 +12:56:17.5
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits
SExtractor catalog cache: saved Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat to cache
SExtractor catalog cache: saved Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.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-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
Creating symlink local_wcs_cache/wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.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-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits exists and is non-empty
wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits exists and is non-empty
wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits exists and is non-empty
wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits exists and is non-empty
The image scale is 5.88"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 13:20:00.311 +13:59:16.89
Second-epoch image center 13:19:54.309 +13:58:22.91
Angular distance between the image centers 0.03 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 13:20:00.311 +13:59:16.89
Second-epoch image center 13:19:51.569 +13:57:59.94
Angular distance between the image centers 0.04 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 13:19:54.309 +13:58:22.91
Second-epoch second image center 13:19:51.569 +13:57:59.94
Angular distance between the image centers 0.01278 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-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits &> /tmp/tmp.k6gYMfzbgs
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits &> /tmp/tmp.ybyRc9FQpx
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits &> /tmp/tmp.hXz2lCr3rU
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits &> /tmp/tmp.PtQVoLRFmk
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.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-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits and wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.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-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits and wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat
Found non-empty wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits and wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat
The reference image (wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits) and catalog (wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat) found
'wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat' -> 'wcsmag.cat'
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
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 3023 out of 30168 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.816035
a=0.000000 b=1.000000 c=22.816035
From vast_summary.log: estimated ref. image limiting mag.: -7.27
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.55
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.55
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 19 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
2.2 pix Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
2.2 pix fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits
2.2 pix fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits
Limiting magnitude estimates:
15.6 mag. Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
15.5 mag. Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
15.3 mag. fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits
15.3 mag. fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits
All-image limiting magnitude estimate: 15.3 (SNR ) 14.7 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.k6gYMfzbgs (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_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.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-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits' -> 'wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
WCS_IMAGE_NAME=wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
WCS-calibrated image found: wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
Checking if the catalog wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat corresponding to the image wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits alredy exist and is non-empty...
Catalog wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat corresponding to the image wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
WCS catalog name: wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=1276, passed=30154
Got 30154 stars (including 28848 good ones) from the SExtractor catalog wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat
util/solve_plate_with_UCAC5 got 30154 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
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...
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.41"
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits -region wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.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.ybyRc9FQpx (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_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.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-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits' -> 'wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
WCS_IMAGE_NAME=wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
WCS-calibrated image found: wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
Checking if the catalog wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits.cat corresponding to the image wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits alredy exist and is non-empty...
Catalog wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits.cat corresponding to the image wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
WCS catalog name: wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=1283, passed=30242
Got 30242 stars (including 28923 good ones) from the SExtractor catalog wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits.cat
util/solve_plate_with_UCAC5 got 30242 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
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...
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.41"
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits -region wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.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.hXz2lCr3rU (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_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.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_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits
WCS_IMAGE_NAME=wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits
WCS-calibrated image found: wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits
Checking if the catalog wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits.cat corresponding to the image wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits.cat corresponding to the image wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits
WCS catalog name: wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=1012, passed=25634
Got 25634 stars (including 24589 good ones) from the SExtractor catalog wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits.cat
util/solve_plate_with_UCAC5 got 25634 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.40"
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits -region wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.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.PtQVoLRFmk (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_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.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_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits
WCS_IMAGE_NAME=wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits
WCS-calibrated image found: wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits
Checking if the catalog wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits.cat corresponding to the image wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits.cat corresponding to the image wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits
WCS catalog name: wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=966, passed=25759
Got 25759 stars (including 24752 good ones) from the SExtractor catalog wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits.cat
util/solve_plate_with_UCAC5 got 25759 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
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...
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.41"
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits -region wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.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-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.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_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/wcs_Vir-01-Q2b1x1_2026-02-22_04-14-54_20.00sec_-15.00C_LIGHT_0415.fits
Saving fully-calibrated image wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.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_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/wcs_Vir-01-Q2b1x1_2026-02-22_04-15-38_20.00sec_-14.90C_LIGHT_0416.fits
Saving fully-calibrated image wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.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_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-49-53_20.00sec_-10.00C_LIGHT_0530.fits
Saving fully-calibrated image wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.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_2026-03-26_CI_Vir-01-Q2b1x1_015453_TTUQ2b1x1_31067_NnC1Zz7j/wcs_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531.fits
Preparing the HTML report for the field Vir-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out51966.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51968.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51971.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51979.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51980.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51981.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51982.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53103.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53480.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53731.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54681.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54688.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54792.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out54135.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54575.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 14s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 51966_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531
The candidate 51966_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531 did not pass the final checks
**** FOUND 13:10:04.16 +14:51:34.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.80, MAG_FAINT_SEARCH_LIMIT=15.78)GAIADR2_OUTPUT=# 0.386 3744032019668958080 197.51738727896 +14.85973268782 15.2547 14.6582 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.386#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51968_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531
The candidate 51968_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531 did not pass the final checks
**** FOUND 13:13:31.29 +18:03:35.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.81, MAG_FAINT_SEARCH_LIMIT=15.79)GAIADR2_OUTPUT=# 4.728 3937266274809484928 198.38165901591 +18.06040099394 14.4311 13.4614 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.728#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51970_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531
The candidate 51970_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531 did not pass the final checks
**** FOUND 13:43:11.39 +13:59:43.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51971_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531
The candidate 51971_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531 did not pass the final checks
**** FOUND 13:14:22.19 +12:08:17.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.79, MAG_FAINT_SEARCH_LIMIT=15.77)GAIADR2_OUTPUT=# 2.368 3736538332529662720 198.59310300373 +12.13832764600 14.8002 13.5089 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.368#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51975_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531
The candidate 51975_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531 did not pass the final checks
**** FOUND 13:42:22.17 +15:29:26.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51979_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531
The candidate 51979_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531 did not pass the final checks
**** FOUND 13:03:23.59 +11:34:37.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)GAIADR2_OUTPUT=# 0.918 3736927044250152192 195.84854179558 +11.57712632563 13.9916 13.4995 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.918#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51980_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531
The candidate 51980_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531 did not pass the final checks
**** FOUND 13:34:19.59 +10:27:54.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 1.511 3726130179366654336 203.58187310036 +10.46550804566 13.7335 13.0234 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.511#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51981_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531
The candidate 51981_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531 did not pass the final checks
**** FOUND 13:15:24.97 +16:43:25.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 0.286 3936874711229704064 198.85408168780 +16.72373591924 13.4466 12.7443 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.286#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51982_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531
The candidate 51982_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531 did not pass the final checks
**** FOUND 13:05:41.43 +12:55:24.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 0.843 3737717696189524736 196.42286202095 +12.92329531191 13.0452 12.2843 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.843#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52514_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531
The candidate 52514_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531 did not pass the final checks
**** FOUND 12:54:50.74 +12:56:17.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53103_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531
The candidate 53103_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531 did not pass the final checks
**** FOUND 13:43:51.91 +13:35:58.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 2.030 3740513273222104576 205.96604921406 +13.60015121830 13.4227 12.8844 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.030#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53480_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531
The candidate 53480_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531 did not pass the final checks
**** FOUND 12:55:35.52 +11:31:24.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 2.807 3735682775044356736 193.89843341434 +11.52418186305 13.6771 13.1563 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.807#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53731_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531
The candidate 53731_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531 did not pass the final checks
**** FOUND 13:21:49.18 +10:44:19.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.05, MAG_FAINT_SEARCH_LIMIT=15.03)GAIADR2_OUTPUT=# 0.495 3733095658544051968 200.45505258014 +10.73882801807 13.9728 13.4422 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.495#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53734_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531
The candidate 53734_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531 did not pass the final checks
**** FOUND 13:10:01.57 +16:10:03.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54135_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531
Preparing report for the candidate 54135_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531
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Considering the candidate 54575_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531
Preparing report for the candidate 54575_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531
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Considering the candidate 54681_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531
The candidate 54681_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531 did not pass the final checks
**** FOUND 13:40:05.98 +14:02:40.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.93, MAG_FAINT_SEARCH_LIMIT=15.91)GAIADR2_OUTPUT=# 1.492 3740762587483759488 205.02532145169 +14.04447823996 14.9177 14.3506 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.492#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54688_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531
The candidate 54688_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531 did not pass the final checks
**** FOUND 13:15:53.07 +11:46:46.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.71, MAG_FAINT_SEARCH_LIMIT=15.69)GAIADR2_OUTPUT=# 0.226 3736466451957027968 198.97109990513 +11.77964110536 14.8110 14.0479 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.226#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54792_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531
The candidate 54792_fd_Vir-01-Q2b1x1_2026-03-26_01-50-41_20.00sec_-10.00C_LIGHT_0531 did not pass the final checks