This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD
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 26.2945* 14 07 23.62 +06 24 30.4 13.0 U Vir 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461125.7945,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260326.2945 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:07:23.62 +06:24:30.4 ;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-05-Q2b1x1_2026-02-22_04-44-54_20_00sec_-14_90C_LIGHT_0446_fits__*pix.png resample_wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20_00sec_-10_00C_LIGHT_0547_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20_00sec_-14_90C_LIGHT_0446_fits__*pix.png resample_wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20_00sec_-10_00C_LIGHT_0546_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20_00sec_-14_90C_LIGHT_0446_fits__*pix.png resample_wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20_00sec_-10_00C_LIGHT_0547_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20_00sec_-14_90C_LIGHT_0446_fits__*pix.png resample_wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20_00sec_-10_00C_LIGHT_0546_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 26.2945* 14 36 36.30 +06 21 43.4 13.2 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,2461125.7945,13.21,0.05,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 20260326.2945 13.21CV 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-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:36:36.30 +06:21:43.4 ;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-05-Q2b1x1_2026-02-22_04-44-54_20_00sec_-14_90C_LIGHT_0446_fits__*pix.png resample_wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20_00sec_-10_00C_LIGHT_0547_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20_00sec_-14_90C_LIGHT_0446_fits__*pix.png resample_wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20_00sec_-10_00C_LIGHT_0546_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20_00sec_-14_90C_LIGHT_0446_fits__*pix.png resample_wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20_00sec_-10_00C_LIGHT_0547_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20_00sec_-14_90C_LIGHT_0446_fits__*pix.png resample_wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20_00sec_-10_00C_LIGHT_0546_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 26.2945* 14 18 36.45 +06 42 16.0 14.3 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,2461125.7945,14.35,0.05,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 20260326.2945 14.35CV 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-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 14:18:36.45 +06:42:16.0 ;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-05-Q2b1x1_2026-02-22_04-44-54_20_00sec_-14_90C_LIGHT_0446_fits__*pix.png resample_wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20_00sec_-10_00C_LIGHT_0547_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20_00sec_-14_90C_LIGHT_0446_fits__*pix.png resample_wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20_00sec_-10_00C_LIGHT_0546_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20_00sec_-14_90C_LIGHT_0446_fits__*pix.png resample_wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20_00sec_-10_00C_LIGHT_0547_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20_00sec_-14_90C_LIGHT_0446_fits__*pix.png resample_wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20_00sec_-10_00C_LIGHT_0546_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: 2461093.94797336 22.02.2026 10:44:54.898 /data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits
First image: 2461093.94797336 22.02.2026 10:44:54.898 /data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits
Last image: 2461125.79472700 26.03.2026 07:04:14.413 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.70
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): 5588
Objects passed selection criteria: 5580
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 5097.5
Average stars matched: 4991.5 (97.9205 %)
Memory usage VmPeak: 112268 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 02:08:59 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: 2461093.94797336 22.02.2026 10:44:54.898 /data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits
First image: 2461093.94797336 22.02.2026 10:44:54.898 /data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits
Last image: 2461125.79472700 26.03.2026 07:04:14.413 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 42
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.38
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 12 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 31921
Objects passed selection criteria: 31865
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 29758.8
Average stars matched: 28701.5 (96.4473 %)
Memory usage VmPeak: 135008 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 02:09:40 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-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits
SExtractor catalog cache: saved Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits.cat to cache
SExtractor catalog cache: saved Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.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-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.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: 2461125.79420347
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-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits exists and is non-empty
Saving wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits to local_wcs_cache/
'wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits' -> 'local_wcs_cache/wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits'
wcs_Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits exists and is non-empty
Saving wcs_Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits to local_wcs_cache/
'wcs_Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits' -> 'local_wcs_cache/wcs_Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits'
wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits exists and is non-empty
Saving wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits to local_wcs_cache/
'wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits' -> 'local_wcs_cache/wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits'
wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits exists and is non-empty
Saving wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits to local_wcs_cache/
'wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits' -> 'local_wcs_cache/wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.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 14:34:31.956 +05:58:42.45
Second-epoch image center 14:34:18.478 +06:00:34.53
Angular distance between the image centers 0.06 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 14:34:31.956 +05:58:42.45
Second-epoch image center 14:34:18.245 +06:00:47.77
Angular distance between the image centers 0.07 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 14:34:18.478 +06:00:34.53
Second-epoch second image center 14:34:18.245 +06:00:47.77
Angular distance between the image centers 0.00380 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-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits &> /tmp/tmp.DvUI25l5L7
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits &> /tmp/tmp.JFrkSDdGjX
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits &> /tmp/tmp.OV67sFZbep
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits &> /tmp/tmp.8DLwGgqbJ7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.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-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits and wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.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-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits and wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits.cat
Found non-empty wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits and wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits.cat
The reference image (wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits) and catalog (wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits.cat) found
'wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.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 3402 out of 7076 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.915381
a=0.000000 b=1.000000 c=22.915381
From vast_summary.log: estimated ref. image limiting mag.: -7.70
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.22
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.22
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.5 pix Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits
2.4 pix Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits
2.4 pix fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits
2.4 pix fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits
Limiting magnitude estimates:
15.2 mag. Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits
15.2 mag. Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits
14.9 mag. fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits
15.0 mag. fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 12.0 (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.DvUI25l5L7 (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-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.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-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits' -> 'wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits
WCS_IMAGE_NAME=wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits
WCS-calibrated image found: wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits
Checking if the catalog wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits.cat corresponding to the image wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits alredy exist and is non-empty...
Catalog wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits.cat corresponding to the image wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits
WCS catalog name: wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=425, passed=7076
Got 7076 stars (including 6645 good ones) from the SExtractor catalog wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits.cat
util/solve_plate_with_UCAC5 got 7076 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 932 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: 0.42"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.42"
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 932 stars left (next iteration limit 1025)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits -region wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.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.JFrkSDdGjX (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-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.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-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits' -> 'wcs_Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits
WCS_IMAGE_NAME=wcs_Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits
WCS-calibrated image found: wcs_Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits
Checking if the catalog wcs_Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits.cat corresponding to the image wcs_Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits alredy exist and is non-empty...
Catalog wcs_Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits.cat corresponding to the image wcs_Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits
WCS catalog name: wcs_Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=431, passed=6892
Got 6892 stars (including 6458 good ones) from the SExtractor catalog wcs_Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits.cat
util/solve_plate_with_UCAC5 got 6892 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 929 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: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.45"
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 929 stars left (next iteration limit 1021)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits -region wcs_Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.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.OV67sFZbep (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-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.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-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits
WCS_IMAGE_NAME=wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits
WCS-calibrated image found: wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits
Checking if the catalog wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits.cat corresponding to the image wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits.cat corresponding to the image wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.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-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits
WCS catalog name: wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=358, passed=5462
Got 5462 stars (including 5099 good ones) from the SExtractor catalog wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits.cat
util/solve_plate_with_UCAC5 got 5462 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 935 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: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.43"
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 935 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits -region wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.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.8DLwGgqbJ7 (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-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.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-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits
WCS_IMAGE_NAME=wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits
WCS-calibrated image found: wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits
Checking if the catalog wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits.cat corresponding to the image wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits.cat corresponding to the image wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.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-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits
WCS catalog name: wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=353, passed=5485
Got 5485 stars (including 5128 good ones) from the SExtractor catalog wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits.cat
util/solve_plate_with_UCAC5 got 5485 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 936 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: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.43"
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 936 stars left (next iteration limit 1029)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits -region wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.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-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits'
Saving fully-calibrated image wcs_Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/wcs_Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits'
Saving fully-calibrated image wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits'
Saving fully-calibrated image wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits'
Preparing the HTML report for the field Vir-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20364.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20221_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547
The candidate 20221_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547 did not pass the final checks
**** FOUND 14:57:48.08 +08:15:34.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20364_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547
The candidate 20364_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547 did not pass the final checks
**** FOUND 14:36:49.66 +06:38:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 0.468 1171444770842163968 219.20704699041 +06.64953870824 12.1486 11.6968 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.468#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06324_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547
The candidate 06324_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547 did not pass the final checks
**** FOUND 14:58:03.30 +09:24:06.0 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Vir-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits
SExtractor catalog cache: saved Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits.cat to cache
SExtractor catalog cache: saved Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.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-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits /data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits
Creating symlink local_wcs_cache/wcs_Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits
Creating symlink local_wcs_cache/wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.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-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits exists and is non-empty
wcs_Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits exists and is non-empty
wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits exists and is non-empty
wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.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 14:34:31.956 +05:58:42.45
Second-epoch image center 14:34:18.478 +06:00:34.53
Angular distance between the image centers 0.06 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 14:34:31.956 +05:58:42.45
Second-epoch image center 14:34:18.245 +06:00:47.77
Angular distance between the image centers 0.07 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 14:34:18.478 +06:00:34.53
Second-epoch second image center 14:34:18.245 +06:00:47.77
Angular distance between the image centers 0.00380 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-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits &> /tmp/tmp.Tjkqx19LmF
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits &> /tmp/tmp.Qt9NsCj894
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits &> /tmp/tmp.WYcPCffv1L
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits &> /tmp/tmp.vLSRWdg2Do
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits
Calibrating the magnitude scale
Found non-empty wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.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-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits and wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.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-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits and wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits.cat
Found non-empty wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits and wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits.cat
The reference image (wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits) and catalog (wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits.cat) found
'wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.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 3418 out of 36795 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.779628
a=0.000000 b=1.000000 c=22.779628
From vast_summary.log: estimated ref. image limiting mag.: -7.38
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.40
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.40
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 32 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits
2.2 pix Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits
2.2 pix fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits
2.2 pix fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits
Limiting magnitude estimates:
15.4 mag. Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits
15.4 mag. Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits
15.1 mag. fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits
15.1 mag. fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 14.5 (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.Tjkqx19LmF (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-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.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-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits' -> 'wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits
WCS_IMAGE_NAME=wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits
WCS-calibrated image found: wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits
Checking if the catalog wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits.cat corresponding to the image wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits alredy exist and is non-empty...
Catalog wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits.cat corresponding to the image wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits
WCS catalog name: wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=1759, passed=36786
Got 36786 stars (including 34984 good ones) from the SExtractor catalog wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits.cat
util/solve_plate_with_UCAC5 got 36786 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 938 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 938 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: 0.38"
Excluding outliers - 938 stars left (next iteration limit 1031)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits -region wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.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.Qt9NsCj894 (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-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.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-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits' -> 'wcs_Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits
WCS_IMAGE_NAME=wcs_Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits
WCS-calibrated image found: wcs_Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits
Checking if the catalog wcs_Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits.cat corresponding to the image wcs_Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits alredy exist and is non-empty...
Catalog wcs_Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits.cat corresponding to the image wcs_Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits
WCS catalog name: wcs_Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=1855, passed=37238
Got 37238 stars (including 35342 good ones) from the SExtractor catalog wcs_Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits.cat
util/solve_plate_with_UCAC5 got 37238 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 934 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: 0.43"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.43"
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 934 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits -region wcs_Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.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.WYcPCffv1L (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-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.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-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits
WCS_IMAGE_NAME=wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits
WCS-calibrated image found: wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits
Checking if the catalog wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits.cat corresponding to the image wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits.cat corresponding to the image wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.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-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits
WCS catalog name: wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=1273, passed=31572
Got 31572 stars (including 30260 good ones) from the SExtractor catalog wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits.cat
util/solve_plate_with_UCAC5 got 31572 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 935 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: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.44"
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 935 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits -region wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.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.vLSRWdg2Do (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-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.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-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits
WCS_IMAGE_NAME=wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits
WCS-calibrated image found: wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits
Checking if the catalog wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits.cat corresponding to the image wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits alredy exist and is non-empty...
Catalog wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits.cat corresponding to the image wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.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-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits
WCS catalog name: wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=1227, passed=31755
Got 31755 stars (including 30479 good ones) from the SExtractor catalog wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits.cat
util/solve_plate_with_UCAC5 got 31755 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 935 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: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.44"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.43"
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 935 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Vir-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits -region wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.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-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.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-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/wcs_Vir-05-Q2b1x1_2026-02-22_04-44-54_20.00sec_-14.90C_LIGHT_0446.fits
Saving fully-calibrated image wcs_Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.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-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/wcs_Vir-05-Q2b1x1_2026-02-22_04-45-38_20.00sec_-15.00C_LIGHT_0447.fits
Saving fully-calibrated image wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.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-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-03-29_20.00sec_-10.00C_LIGHT_0546.fits
Saving fully-calibrated image wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.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-05-Q2b1x1_020648_TTUQ2b1x1_30040_5dcMMzsD/wcs_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547.fits
Preparing the HTML report for the field Vir-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out52640.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52642.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52645.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52646.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52648.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53049.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53187.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53322.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53335.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53435.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53536.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53548.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53550.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53589.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53610.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53621.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53650.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53652.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out52636.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out52965.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52998.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53390.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 52636_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547
The candidate 52636_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547 did not pass the final checks
**** FOUND 14:40:28.73 +06:28:32.8 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.78, MAG_FAINT_SEARCH_LIMIT=15.76)
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Considering the candidate 52640_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547
The candidate 52640_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547 did not pass the final checks
**** FOUND 14:41:46.25 +03:37:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.27, MAG_FAINT_SEARCH_LIMIT=15.25)GAIADR2_OUTPUT=# 1.131 3656562502424950016 220.44277660000 +03.63099879899 14.4355 13.8409 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.131#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52642_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547
The candidate 52642_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547 did not pass the final checks
**** FOUND 14:20:27.12 +06:47:56.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.42, MAG_FAINT_SEARCH_LIMIT=15.40)GAIADR2_OUTPUT=# 2.514 3673361803146616448 215.11339780135 +06.79847975705 14.5123 14.0338 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.514#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52645_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547
The candidate 52645_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547 did not pass the final checks
**** FOUND 14:54:50.28 +09:21:48.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 0.592 1173873012207660544 223.70944335730 +09.36320642070 14.3792 13.7819 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.592#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52646_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547
The candidate 52646_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547 did not pass the final checks
**** FOUND 14:38:06.52 +02:19:21.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.86, MAG_FAINT_SEARCH_LIMIT=14.84)GAIADR2_OUTPUT=# 2.909 3655604827796980352 219.52639459200 +02.32228754693 14.3449 13.8626 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.909#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52648_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547
The candidate 52648_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547 did not pass the final checks
**** FOUND 14:26:45.44 +07:49:05.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)GAIADR2_OUTPUT=# 0.446 1175498502710113024 216.68945754066 +07.81823549860 13.4454 12.7741 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.446#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52650_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547
The candidate 52650_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547 did not pass the final checks
**** FOUND 14:57:48.08 +08:15:34.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52810_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547
The candidate 52810_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 52821_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547
The candidate 52821_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 52849_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547
The candidate 52849_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
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Considering the candidate 52861_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547
The candidate 52861_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
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Considering the candidate 52888_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547
The candidate 52888_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
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Considering the candidate 52965_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547
Preparing report for the candidate 52965_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547
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Considering the candidate 52989_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547
The candidate 52989_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
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Considering the candidate 52998_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547
Preparing report for the candidate 52998_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547
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Considering the candidate 53049_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547
The candidate 53049_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547 did not pass the final checks
**** FOUND 14:34:44.44 +05:30:24.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 0.204 1171219478332831360 218.68519617369 +05.50690955147 13.4770 12.8232 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.204#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53155_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547
The candidate 53155_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547 did not pass the final checks
**** FOUND 14:56:58.38 +04:08:11.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53187_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547
The candidate 53187_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547 did not pass the final checks
**** FOUND 14:35:39.80 +03:27:22.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 2.104 3656682933307794048 218.91620805420 +03.45574523869 13.8917 13.3395 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.104#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53252_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547
The candidate 53252_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
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Considering the candidate 53322_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547
The candidate 53322_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547 did not pass the final checks
**** FOUND 14:48:15.29 +03:19:41.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 3.029 1157552445720464640 222.06317534499 +03.32745940464 14.5465 14.0575 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.029#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53335_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547
The candidate 53335_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547 did not pass the final checks
**** FOUND 14:47:39.74 +09:05:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 1.890 1173709184974832640 221.91609848418 +09.09939826585 14.3476 13.7965 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.890#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53390_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547
Preparing report for the candidate 53390_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547
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Considering the candidate 53421_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547
The candidate 53421_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
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Considering the candidate 53435_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547
The candidate 53435_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547 did not pass the final checks
**** FOUND 14:48:03.80 +04:56:04.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.32, MAG_FAINT_SEARCH_LIMIT=15.30)GAIADR2_OUTPUT=# 1.502 1159131550576238336 222.01569097800 +04.93410775246 14.5176 14.0078 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.502#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53536_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547
The candidate 53536_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547 did not pass the final checks
**** FOUND 14:45:04.62 +03:50:02.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.54, MAG_FAINT_SEARCH_LIMIT=15.52)GAIADR2_OUTPUT=# 2.376 1157831343716805120 221.26879418457 +03.83461729273 15.0422 14.5585 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.376#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53548_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547
The candidate 53548_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547 did not pass the final checks
**** FOUND 14:55:03.08 +06:53:00.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.82, MAG_FAINT_SEARCH_LIMIT=15.80)GAIADR2_OUTPUT=# 0.876 1160922277061034880 223.76285389037 +06.88314634239 14.8377 14.2081 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.876#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53550_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547
The candidate 53550_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547 did not pass the final checks
**** FOUND 14:42:39.98 +03:25:59.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.71, MAG_FAINT_SEARCH_LIMIT=15.69)GAIADR2_OUTPUT=# 0.533 3655793909437345920 220.66660861655 +03.43299295594 14.7570 14.2235 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.533#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53589_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547
The candidate 53589_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547 did not pass the final checks
**** FOUND 14:23:53.10 +05:48:46.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.77, MAG_FAINT_SEARCH_LIMIT=15.75)GAIADR2_OUTPUT=# 1.417 3670181637562072832 215.97164107629 +05.81293951868 14.7365 14.1861 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.417#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53610_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547
The candidate 53610_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547 did not pass the final checks
**** FOUND 14:56:52.90 +04:01:29.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.60, MAG_FAINT_SEARCH_LIMIT=15.58)GAIADR2_OUTPUT=# 1.271 1155029066534641152 224.22050229994 +04.02517590244 14.8498 14.3802 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.271#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53621_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547
The candidate 53621_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547 did not pass the final checks
**** FOUND 14:27:03.45 +08:29:10.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.83, MAG_FAINT_SEARCH_LIMIT=15.81)GAIADR2_OUTPUT=# 1.925 1175676589234075520 216.76485856123 +08.48592732152 14.7184 14.1243 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.925#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53650_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547
The candidate 53650_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547 did not pass the final checks
**** FOUND 14:48:47.75 +09:54:15.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.91, MAG_FAINT_SEARCH_LIMIT=15.89)GAIADR2_OUTPUT=# 1.225 1174891194334649984 222.19900544927 +09.90407946112 15.0343 14.5684 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.225#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53652_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547
The candidate 53652_fd_Vir-05-Q2b1x1_2026-03-26_02-04-14_20.00sec_-10.00C_LIGHT_0547 did not pass the final checks