This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm
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
Gaia DR3 4185055926099795072,2461129.9624,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4185055926099795072 20260330.4624 13.36CV 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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:12:28.18 -15:03:35.7 ;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-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20_00sec_-10_00C_LIGHT_0406_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20_00sec_-10_00C_LIGHT_0405_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20_00sec_-10_00C_LIGHT_0406_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20_00sec_-10_00C_LIGHT_0405_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,2461129.9624,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260330.4624 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:51:45.41 -15:16:03.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20_00sec_-10_00C_LIGHT_0406_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20_00sec_-10_00C_LIGHT_0405_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20_00sec_-10_00C_LIGHT_0406_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20_00sec_-10_00C_LIGHT_0405_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,2461129.9624,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260330.4624 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:14:07.88 -18:04:10.7 ;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-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20_00sec_-10_00C_LIGHT_0406_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20_00sec_-10_00C_LIGHT_0405_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20_00sec_-10_00C_LIGHT_0406_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20_00sec_-10_00C_LIGHT_0405_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: 2461118.99455619 19.03.2026 11:51:59.655 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
First image: 2461118.99455619 19.03.2026 11:51:59.655 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Last image: 2461129.96281792 30.03.2026 11:06:17.468 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.53
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 9869
Objects passed selection criteria: 9866
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 9092
Average stars matched: 8485.25 (93.3266 %)
Memory usage VmPeak: 116500 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 06:08:52 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: 2461118.99455619 19.03.2026 11:51:59.655 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
First image: 2461118.99455619 19.03.2026 11:51:59.655 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Last image: 2461129.96281792 30.03.2026 11:06:17.468 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 66
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.18
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 35 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): 97208
Objects passed selection criteria: 97090
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 94198.2
Average stars matched: 84763.8 (89.9844 %)
Memory usage VmPeak: 1935320 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 06:10:20 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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits
SExtractor catalog cache: saved Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat to cache
SExtractor catalog cache: saved Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.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: 2461129.96201907
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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits exists and is non-empty
Saving wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits to local_wcs_cache/
'wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits' -> 'local_wcs_cache/wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits'
wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits exists and is non-empty
Saving wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits to local_wcs_cache/
'wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits' -> 'local_wcs_cache/wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits'
wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits exists and is non-empty
Saving wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits to local_wcs_cache/
'wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits' -> 'local_wcs_cache/wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits'
wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits exists and is non-empty
Saving wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits to local_wcs_cache/
'wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits' -> 'local_wcs_cache/wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits'
The image scale is 5.88"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 19:33:22.678 -18:00:40.27
Second-epoch image center 19:33:32.729 -18:01:19.39
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 19:33:22.678 -18:00:40.27
Second-epoch image center 19:33:30.050 -18:00:56.87
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 19:33:32.729 -18:01:19.39
Second-epoch second image center 19:33:30.050 -18:00:56.87
Angular distance between the image centers 0.01232 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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits &> /tmp/tmp.3doCGmkkfi
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits &> /tmp/tmp.xcCgpEnbJI
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits &> /tmp/tmp.rc9QqPJqmV
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits &> /tmp/tmp.CGoqfCWowH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits
Calibrating the magnitude scale
Found non-empty wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
Found non-empty wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
The reference image (wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits) and catalog (wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat) found
'wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.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 8546 out of 11017 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.784657
a=0.000000 b=1.000000 c=22.784657
From vast_summary.log: estimated ref. image limiting mag.: -8.53
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.25
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.25
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.5 pix Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
2.0 pix Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
2.5 pix fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits
2.5 pix fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits
Limiting magnitude estimates:
14.3 mag. Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
14.6 mag. Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
13.9 mag. fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits
13.9 mag. fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 11.2 (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.3doCGmkkfi (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits' -> 'wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
WCS_IMAGE_NAME=wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
WCS-calibrated image found: wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Checking if the catalog wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits alredy exist and is non-empty...
Catalog wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
WCS catalog name: wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=800, passed=11017
Got 11017 stars (including 10207 good ones) from the SExtractor catalog wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
util/solve_plate_with_UCAC5 got 11017 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.1'
Seting catalog search parameters based on the expected field of view 938.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013029 (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 0.010423 (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 965 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: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.53"
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 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.53"
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 959 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits -region wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.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.xcCgpEnbJI (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-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.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-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.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-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.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-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits' -> 'wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WCS_IMAGE_NAME=wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WCS-calibrated image found: wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
Checking if the catalog wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits alredy exist and is non-empty...
Catalog wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WCS catalog name: wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1081, passed=13469
Got 13469 stars (including 12369 good ones) from the SExtractor catalog wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat
util/solve_plate_with_UCAC5 got 13469 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 959 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits -region wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.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.rc9QqPJqmV (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-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.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-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits
WCS-calibrated image found: wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits
Checking if the catalog wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.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-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits
WCS catalog name: wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=499, passed=7783
Got 7783 stars (including 7273 good ones) from the SExtractor catalog wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits.cat
util/solve_plate_with_UCAC5 got 7783 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 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.52"
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 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.53"
Estimated accuracy of the plate solution: 0.57"
Excluding outliers - 956 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits -region wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.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.CGoqfCWowH (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-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.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-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits
WCS-calibrated image found: wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits
Checking if the catalog wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.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-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits
WCS catalog name: wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=499, passed=7909
Got 7909 stars (including 7399 good ones) from the SExtractor catalog wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits.cat
util/solve_plate_with_UCAC5 got 7909 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 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.51"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.52"
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits -region wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits'
Saving fully-calibrated image wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits'
Saving fully-calibrated image wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits'
Saving fully-calibrated image wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits'
Preparing the HTML report for the field Sgr-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Sgr-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits
SExtractor catalog cache: saved Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat to cache
SExtractor catalog cache: saved Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Creating symlink local_wcs_cache/wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
Creating symlink local_wcs_cache/wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits
Creating symlink local_wcs_cache/wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits exists and is non-empty
wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits exists and is non-empty
wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits exists and is non-empty
wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits exists and is non-empty
The image scale is 5.88"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 19:33:22.678 -18:00:40.27
Second-epoch image center 19:33:32.729 -18:01:19.39
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 19:33:22.678 -18:00:40.27
Second-epoch image center 19:33:30.050 -18:00:56.87
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 19:33:32.729 -18:01:19.39
Second-epoch second image center 19:33:30.050 -18:00:56.87
Angular distance between the image centers 0.01232 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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits &> /tmp/tmp.6JQat64ElQ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits &> /tmp/tmp.xmlbufHQN0
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits &> /tmp/tmp.NJmAOZL9V3
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits &> /tmp/tmp.PmvHOjFOhi
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits
Calibrating the magnitude scale
Found non-empty wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
Found non-empty wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
The reference image (wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits) and catalog (wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat) found
'wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.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 11996 out of 101850 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.547522
a=0.000000 b=1.000000 c=22.547522
From vast_summary.log: estimated ref. image limiting mag.: -8.18
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.37
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.37
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 53 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
2.0 pix Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
2.3 pix fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits
2.3 pix fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits
Limiting magnitude estimates:
14.4 mag. Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
14.7 mag. Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
14.1 mag. fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits
14.1 mag. fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 13.5 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.6JQat64ElQ (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits' -> 'wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
WCS_IMAGE_NAME=wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
WCS-calibrated image found: wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Checking if the catalog wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits alredy exist and is non-empty...
Catalog wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
WCS catalog name: wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=8404, passed=101839
Got 101839 stars (including 93311 good ones) from the SExtractor catalog wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
util/solve_plate_with_UCAC5 got 101839 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.1'
Seting catalog search parameters based on the expected field of view 938.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013029 (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 0.010423 (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 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.53"
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 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.53"
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 958 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits -region wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.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.xmlbufHQN0 (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-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.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-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.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-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.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-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits' -> 'wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WCS_IMAGE_NAME=wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WCS-calibrated image found: wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
Checking if the catalog wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits alredy exist and is non-empty...
Catalog wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WCS catalog name: wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=12676, passed=138124
Got 138124 stars (including 125221 good ones) from the SExtractor catalog wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat
util/solve_plate_with_UCAC5 got 138124 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (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 964 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: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits -region wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.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.NJmAOZL9V3 (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-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.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-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits
WCS-calibrated image found: wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits
Checking if the catalog wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.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-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits
WCS catalog name: wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=4989, passed=80326
Got 80326 stars (including 75228 good ones) from the SExtractor catalog wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits.cat
util/solve_plate_with_UCAC5 got 80326 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 965 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: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.53"
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 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.53"
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 962 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits -region wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.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.PmvHOjFOhi (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-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.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-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits
WCS-calibrated image found: wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits
Checking if the catalog wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.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-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits
WCS catalog name: wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=5168, passed=81841
Got 81841 stars (including 76570 good ones) from the SExtractor catalog wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits.cat
util/solve_plate_with_UCAC5 got 81841 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 966 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: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.52"
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 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.52"
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Sgr-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits -region wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.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-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Saving fully-calibrated image wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.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-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
Saving fully-calibrated image wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.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-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-05-08_20.00sec_-10.00C_LIGHT_0405.fits
Saving fully-calibrated image wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.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-03-Q2b1x1_060659_TTUQ2b1x1_10773_JSVO8bnm/wcs_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406.fits
Preparing the HTML report for the field Sgr-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out148834.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148835.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148838.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148840.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148842.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148843.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148853.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148855.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148864.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148867.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148873.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148880.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148882.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148885.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148889.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148895.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148897.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148898.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148901.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148908.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148916.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148918.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148966.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149013.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149014.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149022.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149029.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149032.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149095.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149121.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out149137.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out148859.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out149023.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out149039.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: 2s
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Considering the candidate 148834_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 148834_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks
**** FOUND 19:16:32.92 -17:34:02.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 2.615 4084717278096186240 289.13642607366 -17.56761507020 13.5160 12.7332 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.615#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148835_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 148835_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks
**** FOUND 19:39:05.01 -17:30:44.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 1.878 6870196293316146560 294.77032863572 -17.51244204992 13.5894 12.8709 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.878#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148838_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 148838_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks
**** FOUND 19:26:21.33 -17:09:08.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 1.115 4180633278019830656 291.58878713360 -17.15274265582 13.6295 12.9455 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.115#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148840_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 148840_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks
**** FOUND 19:36:00.32 -20:01:15.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 2.557 6869176152684652288 294.00065605115 -20.02134313357 13.6547 12.9710 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.557#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148842_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 148842_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks
**** FOUND 19:15:37.81 -14:00:12.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)
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Considering the candidate 148843_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 148843_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks
**** FOUND 19:23:45.98 -16:53:29.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 2.251 4180799231255038336 290.94096899283 -16.89137046795 13.4847 12.9226 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.251#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148853_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 148853_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks
**** FOUND 19:18:00.84 -15:38:03.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)
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Considering the candidate 148855_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 148855_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks
**** FOUND 19:23:16.87 -15:42:14.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 2.386 4184034823403512832 290.81960370708 -15.70402183687 13.5881 12.9898 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.386#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148859_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
Preparing report for the candidate 148859_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
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Considering the candidate 148864_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 148864_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks
**** FOUND 19:16:00.71 -14:50:17.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 3.482 4185119079311214208 289.00203451320 -14.83845519851 13.2129 12.4754 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.482#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148867_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 148867_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks
**** FOUND 19:36:30.70 -13:50:14.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 2.236 4183196961176903680 294.12731492755 -13.83706713441 13.4299 12.8830 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.236#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148873_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 148873_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks
**** FOUND 19:19:03.80 -15:48:50.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 4.822 4183980328859612160 289.76470857489 -15.81334959529 13.8954 13.2983 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.822#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148878_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 148878_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks
**** FOUND 19:22:52.56 -18:00:30.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148880_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 148880_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks
**** FOUND 19:06:29.35 -15:44:57.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)
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Considering the candidate 148881_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 148881_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks
**** FOUND 19:43:05.41 -18:02:14.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148882_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 148882_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks
**** FOUND 19:10:34.53 -18:00:37.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 4.530 4087267183007556224 287.64508061395 -18.01082394867 13.5046 12.7380 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.530#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148885_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 148885_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks
**** FOUND 19:06:35.03 -16:09:29.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)
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Considering the candidate 148888_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 148888_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks
**** FOUND 19:07:38.46 -13:57:54.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148889_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 148889_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks
**** FOUND 19:10:24.49 -15:40:05.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 0.608 4088952047140303872 287.60190523433 -15.66819962253 12.3539 11.4787 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.608#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148895_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 148895_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks
**** FOUND 19:05:20.14 -14:09:50.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 3.580 4101350616979933824 286.33398597339 -14.16510317133 13.3081 12.5324 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.580#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148897_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 148897_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks
**** FOUND 19:07:38.20 -17:18:32.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)
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Considering the candidate 148898_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 148898_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks
**** FOUND 19:44:36.94 -18:35:44.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 1.404 6869829331310105472 296.15350935383 -18.59558300205 12.7713 12.2328 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.404#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148901_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 148901_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks
**** FOUND 19:09:44.24 -17:12:08.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 0.813 4087885894501201664 287.43455795118 -17.20231863534 12.5373 11.7681 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.813#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148906_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 148906_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks
**** FOUND 19:45:12.95 -15:35:37.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148907_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 148907_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks
**** FOUND 19:15:07.17 -14:49:28.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148908_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 148908_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks
**** FOUND 19:33:53.32 -17:09:43.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 3.178 4180224568930708864 293.47216539315 -17.16106172808 12.6917 11.9202 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.178#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148916_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 148916_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks
**** FOUND 19:30:44.17 -18:54:50.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.89, MAG_FAINT_SEARCH_LIMIT=12.87)GAIADR2_OUTPUT=# 0.236 4179394124111198720 292.68406521326 -18.91411719277 11.9986 11.4298 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.236#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148918_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 148918_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks
**** FOUND 19:15:59.00 -14:26:45.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.18, MAG_FAINT_SEARCH_LIMIT=12.16)GAIADR2_OUTPUT=# 1.395 4185216454811999744 288.99600099048 -14.44632392168 10.8383 10.2717 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.395#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148931_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 148931_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks
**** FOUND 19:17:43.01 -18:55:29.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 148959_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 148959_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks
**** FOUND 19:08:52.25 -18:57:24.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148960_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 148960_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks
**** FOUND 19:36:26.24 -18:52:32.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 148966_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 148966_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks
**** FOUND 19:18:07.59 -18:52:41.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)GAIADR2_OUTPUT=# 2.754 4084282932334862464 289.53094271012 -18.87852159095 12.8322 11.9678 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.754#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148971_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 148971_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks
**** FOUND 19:04:37.25 -21:46:06.1 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 148979_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 148979_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks
**** FOUND 19:26:21.63 -21:14:44.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148983_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 148983_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks
**** FOUND 19:34:17.84 -16:20:40.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148988_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 148988_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks
**** FOUND 19:17:36.64 -15:57:04.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148996_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 148996_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks
**** FOUND 19:24:45.09 -18:37:40.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 149013_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 149013_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks
**** FOUND 19:18:52.45 -19:43:54.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.92, MAG_FAINT_SEARCH_LIMIT=13.90)GAIADR2_OUTPUT=# 3.241 4083067838855425664 289.71864199436 -19.73258980970 12.8047 11.9916 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.241#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149014_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 149014_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks
**** FOUND 19:06:46.85 -21:38:07.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 2.089 4081974821220041216 286.69458636279 -21.63535600793 12.9318 11.8627 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.089#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149015_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 149015_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks
**** FOUND 19:46:26.00 -21:31:41.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 149019_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 149019_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks
**** FOUND 19:37:49.53 -17:12:12.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 149022_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 149022_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks
**** FOUND 19:09:51.15 -20:04:03.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)
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Considering the candidate 149023_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
Preparing report for the candidate 149023_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
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Considering the candidate 149029_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 149029_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks
**** FOUND 19:19:30.96 -21:10:12.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 3.614 4082627656245083520 289.87814968694 -21.16952319343 13.0039 12.1730 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.614#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149032_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 149032_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks
**** FOUND 19:26:42.82 -16:47:38.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 1.911 4180718352733189888 291.67788217021 -16.79416865399 13.0328 12.3117 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.911#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149036_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 149036_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks
**** FOUND 19:30:03.10 -19:22:56.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 149039_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
Preparing report for the candidate 149039_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
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Considering the candidate 149058_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 149058_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks
**** FOUND 19:57:54.02 -15:30:55.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 149061_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 149061_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks
**** FOUND 19:26:17.92 -20:35:44.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 149080_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 149080_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks
**** FOUND 19:29:32.82 -21:19:27.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 149095_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 149095_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks
**** FOUND 19:31:48.00 -18:56:12.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)GAIADR2_OUTPUT=# 2.821 4179379937841129344 292.94920227746 -18.93653850629 13.9579 13.3731 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.821#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149121_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 149121_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks
**** FOUND 19:49:28.18 -18:37:28.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 2.890 6870530476131262976 297.36682361492 -18.62504531033 14.1075 13.5124 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.890#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149137_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406
The candidate 149137_fd_Sgr-03-Q2b1x1_2026-03-30_06-06-17_20.00sec_-10.00C_LIGHT_0406 did not pass the final checks