This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 03 29.3405 2461128.8405 13.20 16:12:28.15 -25:05:24.7
350.28453 18.78104 galactic Sco Second-epoch detections are separated by 4.0" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | EPIC 203745988 | 16:12:27.21 -25:04:51.2 (Gaia DR3) | VAR (local) | 0.307855000000 (local) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
EPIC 203745988,2461128.8405,13.20,0.05,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
EPIC 203745988 20260329.3405 13.20CV 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/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:12:28.15 -25:05:24.7 ;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_Sco-02-Q2b1x1_2026-02-27_05-09-40_20_00sec_-14_90C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20_00sec_-14_90C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20_00sec_-15_00C_LIGHT_0307_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20_00sec_-14_90C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20_00sec_-14_90C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20_00sec_-15_00C_LIGHT_0307_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!
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
ASAS J161332-2655.8,2461128.8405,12.49,0.05,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
ASAS J161332-2655.8 20260329.3405 12.49CV 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/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:13:31.76 -26:55:46.9 ;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_Sco-02-Q2b1x1_2026-02-27_05-09-40_20_00sec_-14_90C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20_00sec_-14_90C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20_00sec_-15_00C_LIGHT_0307_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20_00sec_-14_90C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20_00sec_-14_90C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20_00sec_-15_00C_LIGHT_0307_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!
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
ZZ Sco,2461128.8405,12.52,0.05,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
ZZ Sco 20260329.3405 12.52CV 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/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:41:01.00 -27:26:45.1 ;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_Sco-02-Q2b1x1_2026-02-27_05-09-40_20_00sec_-14_90C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20_00sec_-14_90C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20_00sec_-15_00C_LIGHT_0307_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20_00sec_-14_90C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20_00sec_-14_90C_LIGHT_0010_fits__*pix.png resample_wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20_00sec_-15_00C_LIGHT_0307_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: 2461098.96517225 27.02.2026 11:09:40.882 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
First image: 2461098.96517225 27.02.2026 11:09:40.882 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
Last image: 2461128.84079289 29.03.2026 08:10:34.506 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.21
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 6218
Objects passed selection criteria: 6203
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 5218.75
Average stars matched: 5089.75 (97.5281 %)
Memory usage VmPeak: 113188 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 Sun Mar 29 03:12:41 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.96517225 27.02.2026 11:09:40.882 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
First image: 2461098.96517225 27.02.2026 11:09:40.882 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
Last image: 2461128.84079289 29.03.2026 08:10:34.506 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 56
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.89
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 15 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): 62906
Objects passed selection criteria: 62815
Measurements per detected object (mean, median, min, max): 3.1 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 3.0 2 4
Average stars detected per image: 51454.8
Average stars matched: 49835 (96.8521 %)
Memory usage VmPeak: 168600 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 Sun Mar 29 03:13:45 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/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits
SExtractor catalog cache: saved Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat to cache
SExtractor catalog cache: saved Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.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/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.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: 2461128.84017191
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits exists and is non-empty
Saving wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits to local_wcs_cache/
'wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits' -> 'local_wcs_cache/wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits'
wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits exists and is non-empty
Saving wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits to local_wcs_cache/
'wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits' -> 'local_wcs_cache/wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits'
wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits exists and is non-empty
Saving wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits to local_wcs_cache/
'wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits' -> 'local_wcs_cache/wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits'
wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits exists and is non-empty
Saving wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits to local_wcs_cache/
'wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits' -> 'local_wcs_cache/wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:19:16.444 -25:59:35.75
Second-epoch image center 16:19:10.633 -26:01:15.58
Angular distance between the image centers 0.04 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 16:19:16.444 -25:59:35.75
Second-epoch image center 16:19:07.758 -26:01:20.13
Angular distance between the image centers 0.04 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 16:19:10.633 -26:01:15.58
Second-epoch second image center 16:19:07.758 -26:01:20.13
Angular distance between the image centers 0.01084 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/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits &> /tmp/tmp.tjXopuGG7f
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits &> /tmp/tmp.cw1sqmwqt2
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits &> /tmp/tmp.jGRkomov4j
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits &> /tmp/tmp.uoETUOnv1q
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits
Calibrating the magnitude scale
Found non-empty wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.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_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits and wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.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_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits and wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat
Found non-empty wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits and wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat
The reference image (wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits) and catalog (wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat) found
'wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.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 5823 out of 8752 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.788280
a=0.000000 b=1.000000 c=22.788280
From vast_summary.log: estimated ref. image limiting mag.: -8.21
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.58
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.58
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
2.2 pix Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
2.9 pix fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits
2.9 pix fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits
Limiting magnitude estimates:
14.6 mag. Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
14.6 mag. Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
13.8 mag. fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits
13.8 mag. fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 11.1 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.tjXopuGG7f (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits' -> 'wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
WCS_IMAGE_NAME=wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
WCS-calibrated image found: wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
Checking if the catalog wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat corresponding to the image wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits alredy exist and is non-empty...
Catalog wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat corresponding to the image wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
WCS catalog name: wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=696, passed=8752
Got 8752 stars (including 8042 good ones) from the SExtractor catalog wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat
util/solve_plate_with_UCAC5 got 8752 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 963 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: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits -region wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.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.cw1sqmwqt2 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits' -> 'wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
WCS_IMAGE_NAME=wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
WCS-calibrated image found: wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
Checking if the catalog wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat corresponding to the image wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits alredy exist and is non-empty...
Catalog wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat corresponding to the image wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
WCS catalog name: wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=689, passed=8852
Got 8852 stars (including 8148 good ones) from the SExtractor catalog wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat
util/solve_plate_with_UCAC5 got 8852 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 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: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits -region wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.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.jGRkomov4j (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_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.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_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits
WCS_IMAGE_NAME=wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits
WCS-calibrated image found: wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits
Checking if the catalog wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits.cat corresponding to the image wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits.cat corresponding to the image wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits
WCS catalog name: wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=345, passed=4640
Got 4640 stars (including 4292 good ones) from the SExtractor catalog wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits.cat
util/solve_plate_with_UCAC5 got 4640 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (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 0.010422 (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 959 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: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.66"
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 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.67"
Estimated accuracy of the plate solution: 0.73"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits -region wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.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.uoETUOnv1q (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_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.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_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits
WCS_IMAGE_NAME=wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits
WCS-calibrated image found: wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits
Checking if the catalog wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits.cat corresponding to the image wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits.cat corresponding to the image wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits
WCS catalog name: wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=331, passed=4675
Got 4675 stars (including 4338 good ones) from the SExtractor catalog wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits.cat
util/solve_plate_with_UCAC5 got 4675 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (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 0.010422 (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 957 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: 0.64"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.65"
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 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.67"
Estimated accuracy of the plate solution: 0.72"
Excluding outliers - 955 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits -region wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.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_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits'
Saving fully-calibrated image wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits'
Saving fully-calibrated image wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits'
Saving fully-calibrated image wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits'
Preparing the HTML report for the field Sco-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
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: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20490_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 20490_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks
**** FOUND 16:24:09.30 -28:22:22.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01392_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 01392_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks
**** FOUND 16:00:42.42 -29:55:16.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03020_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 03020_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks
**** FOUND 16:38:12.86 -28:34:09.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06191_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 06191_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks
**** FOUND 16:11:57.15 -24:53:57.4 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 0s
Prepared the HTML report for the field Sco-02-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/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits
SExtractor catalog cache: saved Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat to cache
SExtractor catalog cache: saved Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
Creating symlink local_wcs_cache/wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
Creating symlink local_wcs_cache/wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits
Creating symlink local_wcs_cache/wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.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_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits exists and is non-empty
wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits exists and is non-empty
wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits exists and is non-empty
wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:19:16.444 -25:59:35.75
Second-epoch image center 16:19:10.633 -26:01:15.58
Angular distance between the image centers 0.04 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 16:19:16.444 -25:59:35.75
Second-epoch image center 16:19:07.758 -26:01:20.13
Angular distance between the image centers 0.04 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 16:19:10.633 -26:01:15.58
Second-epoch second image center 16:19:07.758 -26:01:20.13
Angular distance between the image centers 0.01084 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/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits &> /tmp/tmp.uoHHAF5HUl
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits &> /tmp/tmp.MAKJ5T9cge
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits &> /tmp/tmp.jfUqfmayf0
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits &> /tmp/tmp.7cDLSzJ9yt
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits
Calibrating the magnitude scale
Found non-empty wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.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_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits and wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.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_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits and wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat
Found non-empty wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits and wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat
The reference image (wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits) and catalog (wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat) found
'wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.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 6991 out of 85371 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.596036
a=0.000000 b=1.000000 c=22.596036
From vast_summary.log: estimated ref. image limiting mag.: -7.89
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.71
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.71
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 49 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
2.0 pix Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
2.4 pix fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits
2.5 pix fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits
Limiting magnitude estimates:
14.7 mag. Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
14.7 mag. Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
13.9 mag. fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits
13.9 mag. fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 13.3 (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.uoHHAF5HUl (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits' -> 'wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
WCS_IMAGE_NAME=wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
WCS-calibrated image found: wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
Checking if the catalog wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat corresponding to the image wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits alredy exist and is non-empty...
Catalog wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat corresponding to the image wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
WCS catalog name: wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=4769, passed=85367
Got 85367 stars (including 80428 good ones) from the SExtractor catalog wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat
util/solve_plate_with_UCAC5 got 85367 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits -region wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.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.MAKJ5T9cge (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits' -> 'wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
WCS_IMAGE_NAME=wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
WCS-calibrated image found: wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
Checking if the catalog wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat corresponding to the image wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits alredy exist and is non-empty...
Catalog wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat corresponding to the image wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
WCS catalog name: wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=4773, passed=84610
Got 84610 stars (including 79676 good ones) from the SExtractor catalog wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat
util/solve_plate_with_UCAC5 got 84610 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits -region wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.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.jfUqfmayf0 (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_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.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_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits
WCS_IMAGE_NAME=wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits
WCS-calibrated image found: wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits
Checking if the catalog wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits.cat corresponding to the image wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits.cat corresponding to the image wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits
WCS catalog name: wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=1988, passed=38497
Got 38497 stars (including 36468 good ones) from the SExtractor catalog wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits.cat
util/solve_plate_with_UCAC5 got 38497 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (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 0.010422 (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 960 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: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.59"
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 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.59"
Estimated accuracy of the plate solution: 0.66"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits -region wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.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.7cDLSzJ9yt (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_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.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_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits
WCS_IMAGE_NAME=wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits
WCS-calibrated image found: wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits
Checking if the catalog wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits.cat corresponding to the image wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits.cat corresponding to the image wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits
WCS catalog name: wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=1939, passed=38689
Got 38689 stars (including 36706 good ones) from the SExtractor catalog wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits.cat
util/solve_plate_with_UCAC5 got 38689 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.0'
Seting catalog search parameters based on the expected field of view 938.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013028 (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 0.010422 (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 961 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: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.60"
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 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.60"
Estimated accuracy of the plate solution: 0.66"
Excluding outliers - 959 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits -region wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.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_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.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_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
Saving fully-calibrated image wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.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_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
Saving fully-calibrated image wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.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_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-09-40_20.00sec_-15.00C_LIGHT_0307.fits
Saving fully-calibrated image wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.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_2026-03-29_CI_Sco-02-Q2b1x1_031117_TTUQ2b1x1_15149_cTQ6x14p/wcs_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308.fits
Preparing the HTML report for the field Sco-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out101588.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out101590.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out101701.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out101748.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37457.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41875.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 10s
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 101582_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 101582_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 101588_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 101588_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks
**** FOUND 16:19:23.13 -21:53:03.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 0.825 6052090162559893376 244.84629909424 -21.88403190641 12.2906 11.7557 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.825#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 101590_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 101590_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks
**** FOUND 16:11:24.19 -25:54:03.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)
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Considering the candidate 101624_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 101624_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks
**** FOUND 16:23:39.79 -26:28:50.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101626_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 101626_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks
**** FOUND 16:23:21.39 -26:31:08.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101628_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 101628_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks
**** FOUND 16:23:21.98 -26:30:49.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101635_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 101635_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks
**** FOUND 16:08:02.91 -26:17:27.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101638_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 101638_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks
**** FOUND 16:23:24.09 -26:30:18.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101647_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 101647_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
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Considering the candidate 101651_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 101651_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks
**** FOUND 16:21:00.20 -25:36:03.9 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 101654_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 101654_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks
**** FOUND 16:23:30.28 -26:29:44.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101659_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 101659_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks
**** FOUND 16:23:24.59 -26:32:23.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101660_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 101660_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks
**** FOUND 16:36:11.61 -24:47:44.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101668_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 101668_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks
**** FOUND 16:23:42.51 -26:29:31.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101677_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 101677_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks
**** FOUND 16:23:21.11 -26:31:38.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101684_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 101684_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks
**** FOUND 16:07:52.07 -24:29:06.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 101693_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 101693_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks
**** FOUND 16:23:21.27 -26:31:59.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101701_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 101701_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks
**** FOUND 15:56:45.38 -23:11:56.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 1.743 6237347121542276608 239.18860490565 -23.19909158535 12.6183 11.8403 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.743#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 101702_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 101702_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks
**** FOUND 16:38:02.75 -25:08:30.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101708_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 101708_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks
**** FOUND 16:23:24.97 -26:31:48.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101711_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 101711_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks
**** FOUND 15:50:35.85 -23:14:58.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101718_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 101718_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks
**** FOUND 16:23:35.64 -26:28:36.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101721_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 101721_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks
**** FOUND 16:04:38.41 -24:05:25.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101727_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 101727_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks
**** FOUND 16:05:42.77 -21:49:24.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101728_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 101728_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks
**** FOUND 16:08:01.84 -26:18:03.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 101733_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 101733_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks
**** FOUND 16:38:57.81 -27:25:26.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101741_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 101741_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks
**** FOUND 16:31:31.15 -26:10:21.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101748_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
Preparing report for the candidate 101748_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
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Considering the candidate 101752_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 101752_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks
**** FOUND 16:09:34.76 -27:53:42.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101758_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 101758_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks
**** FOUND 16:02:42.69 -26:54:37.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101763_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 101763_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks
**** FOUND 16:42:48.28 -24:18:08.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 76483_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 76483_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks
**** FOUND 16:26:39.25 -22:19:00.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 13364_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 13364_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks
**** FOUND 16:23:16.40 -29:56:03.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58926_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 58926_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks
**** FOUND 16:42:01.73 -25:02:07.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 42207_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 42207_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks
**** FOUND 16:40:48.59 -26:55:14.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 69181_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 69181_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks
**** FOUND 16:17:40.51 -22:53:38.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 41875_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
Preparing report for the candidate 41875_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
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Considering the candidate 59113_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 59113_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks
**** FOUND 16:11:57.14 -24:53:57.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 74688_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 74688_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks
**** FOUND 15:58:46.54 -21:49:47.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 47430_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 47430_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks
**** FOUND 16:23:31.96 -26:24:21.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 11594_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 11594_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks
**** FOUND 16:00:42.41 -29:55:16.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57579_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 57579_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks
**** FOUND 16:09:51.77 -25:08:42.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33479_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 33479_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks
**** FOUND 16:31:40.87 -27:54:36.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 28999_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 28999_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks
**** FOUND 16:24:09.30 -28:22:22.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 37457_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
Preparing report for the candidate 37457_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
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Considering the candidate 79343_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 79343_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks
**** FOUND 16:18:05.45 -21:49:05.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67931_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 67931_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks
**** FOUND 16:03:35.13 -22:41:12.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 37555_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 37555_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks
**** FOUND 16:46:34.81 -27:23:15.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 26638_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308
The candidate 26638_fd_Sco-02-Q2b1x1_2026-03-29_03-10-34_20.00sec_-15.00C_LIGHT_0308 did not pass the final checks