This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461129.8889,10.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260330.3889 10.72CV 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/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:51:25.41 -19:02:51.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20_00sec_-10_00C_LIGHT_0336_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20_00sec_-10_00C_LIGHT_0335_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20_00sec_-10_00C_LIGHT_0336_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20_00sec_-10_00C_LIGHT_0335_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
VARIABLE_NAME,2461129.8889,13.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260330.3889 13.69CV 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/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 17:57:37.16 -16:46:34.7 ;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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20_00sec_-10_00C_LIGHT_0336_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20_00sec_-10_00C_LIGHT_0335_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20_00sec_-10_00C_LIGHT_0336_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20_00sec_-15_00C_LIGHT_0061_fits__*pix.png resample_wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20_00sec_-10_00C_LIGHT_0335_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: 2461099.00589001 27.02.2026 12:08:18.897 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
First image: 2461099.00589001 27.02.2026 12:08:18.897 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
Last image: 2461129.88915880 30.03.2026 09:20:13.320 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.23
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 10020
Objects passed selection criteria: 9996
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 7635.25
Average stars matched: 7441.75 (97.4657 %)
Memory usage VmPeak: 117364 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 Mon Mar 30 04:24:44 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: 2461099.00589001 27.02.2026 12:08:18.897 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
First image: 2461099.00589001 27.02.2026 12:08:18.897 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
Last image: 2461129.88915880 30.03.2026 09:20:13.320 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 77
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.87
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: 31 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): 134057
Objects passed selection criteria: 133738
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 104217
Average stars matched: 99503.2 (95.4768 %)
Memory usage VmPeak: 1974984 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 Mon Mar 30 04:28:02 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/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits
SExtractor catalog cache: saved Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat to cache
SExtractor catalog cache: saved Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.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/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.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: 2461129.88855956
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits exists and is non-empty
Saving wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits to local_wcs_cache/
'wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits' -> 'local_wcs_cache/wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits'
wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits exists and is non-empty
Saving wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits to local_wcs_cache/
'wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits' -> 'local_wcs_cache/wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits'
wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits exists and is non-empty
Saving wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits to local_wcs_cache/
'wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits' -> 'local_wcs_cache/wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits'
wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits exists and is non-empty
Saving wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits to local_wcs_cache/
'wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits' -> 'local_wcs_cache/wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.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 17:46:18.174 -18:00:45.70
Second-epoch image center 17:46:27.989 -18:00:29.00
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 17:46:18.174 -18:00:45.70
Second-epoch image center 17:46:25.408 -18:00:05.95
Angular distance between the image centers 0.03 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 17:46:27.989 -18:00:29.00
Second-epoch second image center 17:46:25.408 -18:00:05.95
Angular distance between the image centers 0.01207 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/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits &> /tmp/tmp.K73JUsOLyh
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits &> /tmp/tmp.Qcski7sG2r
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits &> /tmp/tmp.UgC6LT7GiJ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits &> /tmp/tmp.TFpJe1cCJU
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits
Calibrating the magnitude scale
Found non-empty wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits and wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits and wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat
Found non-empty wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits and wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat
The reference image (wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits) and catalog (wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat) found
'wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.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 10414 out of 15752 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.846952
a=0.000000 b=1.000000 c=22.846952
From vast_summary.log: estimated ref. image limiting mag.: -8.23
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.62
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.62
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
2.3 pix Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
2.6 pix fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits
2.5 pix fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits
Limiting magnitude estimates:
14.6 mag. Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
14.6 mag. Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
13.6 mag. fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits
13.6 mag. fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits
All-image limiting magnitude estimate: 13.6 (SNR ) 10.9 (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.K73JUsOLyh (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/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.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_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits' -> 'wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
WCS_IMAGE_NAME=wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
WCS-calibrated image found: wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
Checking if the catalog wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat corresponding to the image wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits alredy exist and is non-empty...
Catalog wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat corresponding to the image wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
WCS catalog name: wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1456, passed=15752
Got 15752 stars (including 14271 good ones) from the SExtractor catalog wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat
util/solve_plate_with_UCAC5 got 15752 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 919 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: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 918 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.37"
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 914 stars left (next iteration limit 1006)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits -region wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.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.Qcski7sG2r (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/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.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_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits' -> 'wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
WCS_IMAGE_NAME=wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
WCS-calibrated image found: wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
Checking if the catalog wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat corresponding to the image wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits alredy exist and is non-empty...
Catalog wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat corresponding to the image wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
WCS catalog name: wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1474, passed=15602
Got 15602 stars (including 14101 good ones) from the SExtractor catalog wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat
util/solve_plate_with_UCAC5 got 15602 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 919 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
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 918 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.39"
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 915 stars left (next iteration limit 1007)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits -region wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.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.UgC6LT7GiJ (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_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.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_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits
WCS-calibrated image found: wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits
Checking if the catalog wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits.cat corresponding to the image wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits.cat corresponding to the image wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits
WCS catalog name: wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=429, passed=6229
Got 6229 stars (including 5796 good ones) from the SExtractor catalog wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits.cat
util/solve_plate_with_UCAC5 got 6229 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 922 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: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.71"
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 922 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.72"
Estimated accuracy of the plate solution: 0.78"
Excluding outliers - 917 stars left (next iteration limit 1009)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits -region wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.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.TFpJe1cCJU (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_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.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_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits
WCS-calibrated image found: wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits
Checking if the catalog wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits.cat corresponding to the image wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits.cat corresponding to the image wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits
WCS catalog name: wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=459, passed=6238
Got 6238 stars (including 5770 good ones) from the SExtractor catalog wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits.cat
util/solve_plate_with_UCAC5 got 6238 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 919 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: 0.70"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.74"
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 919 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.75"
Estimated accuracy of the plate solution: 0.81"
Excluding outliers - 915 stars left (next iteration limit 1006)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits -region wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits'
Saving fully-calibrated image wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits'
Saving fully-calibrated image wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits'
Saving fully-calibrated image wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits'
Preparing the HTML report for the field Sgr-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out20763.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20763_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
Preparing report for the candidate 20763_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 6s
Prepared the HTML report for the field Sgr-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
17:51:25.41 -19:02:51.3
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits
SExtractor catalog cache: saved Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat to cache
SExtractor catalog cache: saved Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
Creating symlink local_wcs_cache/wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
Creating symlink local_wcs_cache/wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits
Creating symlink local_wcs_cache/wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits exists and is non-empty
wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits exists and is non-empty
wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits exists and is non-empty
wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.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 17:46:18.174 -18:00:45.70
Second-epoch image center 17:46:27.989 -18:00:29.00
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 17:46:18.174 -18:00:45.70
Second-epoch image center 17:46:25.408 -18:00:05.95
Angular distance between the image centers 0.03 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 17:46:27.989 -18:00:29.00
Second-epoch second image center 17:46:25.408 -18:00:05.95
Angular distance between the image centers 0.01207 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/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits &> /tmp/tmp.BUSA4ANfY3
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits &> /tmp/tmp.8V6VYsRsyv
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits &> /tmp/tmp.5TCVsnymLf
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits &> /tmp/tmp.hMkhzHnBxR
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits
Calibrating the magnitude scale
Found non-empty wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits and wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits and wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat
Found non-empty wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits and wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat
The reference image (wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits) and catalog (wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat) found
'wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.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 12785 out of 179796 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.613163
a=0.000000 b=1.000000 c=22.613163
From vast_summary.log: estimated ref. image limiting mag.: -7.87
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.74
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.74
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 56 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
1.9 pix Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
2.3 pix fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits
2.2 pix fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits
Limiting magnitude estimates:
14.7 mag. Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
14.7 mag. Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
13.7 mag. fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits
13.8 mag. fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits
All-image limiting magnitude estimate: 13.7 (SNR ) 13.2 (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.BUSA4ANfY3 (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/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.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_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits' -> 'wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
WCS_IMAGE_NAME=wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
WCS-calibrated image found: wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
Checking if the catalog wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat corresponding to the image wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits alredy exist and is non-empty...
Catalog wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat corresponding to the image wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
WCS catalog name: wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=28, blended=17851, passed=179768
Got 179768 stars (including 161620 good ones) from the SExtractor catalog wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat
util/solve_plate_with_UCAC5 got 179768 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 923 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 923 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.41"
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 919 stars left (next iteration limit 1012)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits -region wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.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.8V6VYsRsyv (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/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.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_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits' -> 'wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
WCS_IMAGE_NAME=wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
WCS-calibrated image found: wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
Checking if the catalog wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat corresponding to the image wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits alredy exist and is non-empty...
Catalog wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat corresponding to the image wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
WCS catalog name: wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=17987, passed=181054
Got 181054 stars (including 162799 good ones) from the SExtractor catalog wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat
util/solve_plate_with_UCAC5 got 181054 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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 925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
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 924 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.45"
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 921 stars left (next iteration limit 1013)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits -region wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.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.5TCVsnymLf (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_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.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_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits
WCS-calibrated image found: wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits
Checking if the catalog wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits.cat corresponding to the image wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits.cat corresponding to the image wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits
WCS catalog name: wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=3586, passed=67028
Got 67028 stars (including 63384 good ones) from the SExtractor catalog wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits.cat
util/solve_plate_with_UCAC5 got 67028 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 924 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: 0.65"
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 924 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.61"
Estimated accuracy of the plate solution: 0.66"
Excluding outliers - 917 stars left (next iteration limit 1009)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits -region wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.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.hMkhzHnBxR (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_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.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_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits
WCS-calibrated image found: wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits
Checking if the catalog wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits.cat corresponding to the image wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits.cat corresponding to the image wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits
WCS catalog name: wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=1, no_mag_err=0, low_SNR=6, blended=3816, passed=69467
Got 69467 stars (including 65572 good ones) from the SExtractor catalog wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits.cat
util/solve_plate_with_UCAC5 got 69467 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 923 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: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.63"
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 923 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.63"
Estimated accuracy of the plate solution: 0.68"
Excluding outliers - 919 stars left (next iteration limit 1010)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits -region wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.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_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
Saving fully-calibrated image wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.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_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
Saving fully-calibrated image wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.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_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-19-21_20.00sec_-10.00C_LIGHT_0335.fits
Saving fully-calibrated image wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.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_2026-03-30_CI_Sgr-01-Q2b1x1_042059_TTUQ2b1x1_28289_TRYKL7sK/wcs_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336.fits
Preparing the HTML report for the field Sgr-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out208313.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208320.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208325.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208330.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208337.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208338.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208340.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208342.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208354.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208357.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208361.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208366.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208388.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208393.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208462.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208477.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out208535.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208313_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 208313_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 17:37:41.38 -14:11:29.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208320_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 208320_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 17:27:55.71 -17:03:27.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208325_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 208325_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 17:52:48.31 -15:57:29.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 2.450 4147992381267589632 268.20151530797 -15.95870137342 12.8358 11.7593 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.450#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208329_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 208329_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 17:38:07.35 -17:25:54.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208330_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 208330_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 17:53:09.35 -17:59:59.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 0.358 4120440166057276800 268.28905303305 -17.99995888862 13.3734 12.7595 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.358#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208337_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 208337_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 17:32:17.18 -16:32:49.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208338_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 208338_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 18:03:12.85 -20:18:44.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208340_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 208340_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 17:55:54.62 -19:24:53.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208342_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 208342_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 18:04:00.62 -19:48:45.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 1.196 4095191049755546240 271.00244249131 -19.81297126208 12.6123 11.5250 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.196#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208348_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 208348_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 17:55:54.73 -15:35:42.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208354_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 208354_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 18:03:17.91 -19:47:27.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 2.871 4095193489296330112 270.82532637276 -19.79150339421 12.5770 11.5523 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.871#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208357_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 208357_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 17:52:17.24 -18:04:38.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 3.741 4120432920551392512 268.07107106041 -18.07653295420 12.4344 11.1782 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.741#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208361_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 208361_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 17:46:02.52 -16:12:04.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 0.369 4148100103400650752 266.51040939152 -16.20119573831 12.9348 12.2658 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.369#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208362_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 208362_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 18:09:21.43 -14:16:23.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208366_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 208366_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 18:12:04.40 -19:21:03.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208370_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 208370_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 17:39:17.96 -17:48:28.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208376_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 208376_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 18:10:34.06 -15:42:12.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208383_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 208383_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 18:05:40.74 -15:27:46.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208384_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 208384_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 18:09:18.64 -18:16:55.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208387_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 208387_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 18:08:22.48 -14:22:33.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208388_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 208388_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 17:43:19.20 -14:59:45.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.93, MAG_FAINT_SEARCH_LIMIT=12.91)GAIADR2_OUTPUT=# 0.380 4149047706266318976 265.83002493858 -14.99615843686 11.6495 10.6950 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.380#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208389_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 208389_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 18:03:50.69 -15:32:04.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208391_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 208391_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 18:06:19.49 -16:41:16.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208392_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 208392_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 18:12:03.46 -17:38:52.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208393_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 208393_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 17:26:24.01 -19:31:22.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.34, MAG_FAINT_SEARCH_LIMIT=11.32)GAIADR2_OUTPUT=# 1.408 4121355479493298176 261.60040628336 -19.52296442750 10.3393 9.7685 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.408#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208405_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 208405_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 17:51:25.42 -19:02:51.5 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208453_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 208453_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 18:11:40.75 -14:26:53.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208457_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 208457_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 18:01:12.82 -15:19:54.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208462_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 208462_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 17:17:32.74 -17:53:44.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 4.982 4134571437428355200 259.38575438247 -17.89703752228 12.4608 11.7074 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.982#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208464_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 208464_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 17:29:59.48 -17:21:54.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208466_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 208466_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 18:01:28.61 -17:09:38.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208468_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 208468_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 17:59:25.84 -15:09:14.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208474_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 208474_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 18:10:45.09 -16:29:33.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208477_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 208477_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 18:00:42.50 -17:21:11.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 0.571 4143848738654464896 270.17722327288 -17.35316446291 12.7705 11.8311 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.571#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208482_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 208482_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 17:46:07.88 -21:35:21.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208483_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 208483_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 17:25:59.50 -14:03:14.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208485_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 208485_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 18:11:10.86 -15:11:24.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208507_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 208507_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 18:02:54.04 -14:31:50.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208508_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 208508_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208517_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 208517_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 17:56:25.70 -16:13:46.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208525_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 208525_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 17:44:10.88 -18:35:47.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208529_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 208529_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 17:25:14.50 -18:35:26.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208535_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
Preparing report for the candidate 208535_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190967_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 190967_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 17:31:55.91 -19:19:43.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 44480_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 44480_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 17:21:49.40 -19:58:58.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111310_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 111310_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 17:48:11.35 -16:47:18.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197834_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 197834_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 17:56:17.18 -16:53:25.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191701_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 191701_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 18:02:38.56 -22:12:15.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 90291_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 90291_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 17:29:56.23 -17:40:40.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33957_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 33957_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 17:20:58.88 -20:38:46.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136842_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 136842_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 18:02:00.66 -15:16:31.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60437_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 60437_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 17:38:29.52 -19:05:54.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 49659_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 49659_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 17:24:39.61 -19:39:41.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195040_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 195040_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 17:43:29.48 -14:52:27.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 175775_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 175775_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks
**** FOUND 17:21:15.26 -14:38:04.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25679_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336
The candidate 25679_fd_Sgr-01-Q2b1x1_2026-03-30_04-20-13_20.00sec_-10.00C_LIGHT_0336 did not pass the final checks