This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461121.7967,10.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260322.2967 10.85CV 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/Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:34:36.19 +28:41:52.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20_00sec_-15_00C_LIGHT_0662_fits__*pix.png resample_wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20_00sec_-14_90C_LIGHT_0154_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20_00sec_-15_00C_LIGHT_0662_fits__*pix.png resample_wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20_00sec_-15_00C_LIGHT_0153_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20_00sec_-15_00C_LIGHT_0662_fits__*pix.png resample_wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20_00sec_-14_90C_LIGHT_0154_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20_00sec_-15_00C_LIGHT_0662_fits__*pix.png resample_wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20_00sec_-15_00C_LIGHT_0153_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.2967* 09 38 46.90 +27 28 05.3 13.6 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461121.7967,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260322.2967 13.62CV 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/Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:38:46.90 +27:28:05.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20_00sec_-15_00C_LIGHT_0662_fits__*pix.png resample_wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20_00sec_-14_90C_LIGHT_0154_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20_00sec_-15_00C_LIGHT_0662_fits__*pix.png resample_wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20_00sec_-15_00C_LIGHT_0153_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20_00sec_-15_00C_LIGHT_0662_fits__*pix.png resample_wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20_00sec_-14_90C_LIGHT_0154_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20_00sec_-15_00C_LIGHT_0662_fits__*pix.png resample_wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20_00sec_-15_00C_LIGHT_0153_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.2967* 09 46 49.66 +26 39 13.4 13.9 U Leo 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461121.7967,13.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260322.2967 13.91CV 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/Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:46:49.66 +26:39:13.4 ;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_Leo-01-Q1b1x1_2025-12-23_06-02-07_20_00sec_-15_00C_LIGHT_0662_fits__*pix.png resample_wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20_00sec_-14_90C_LIGHT_0154_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20_00sec_-15_00C_LIGHT_0662_fits__*pix.png resample_wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20_00sec_-15_00C_LIGHT_0153_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20_00sec_-15_00C_LIGHT_0662_fits__*pix.png resample_wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20_00sec_-14_90C_LIGHT_0154_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20_00sec_-15_00C_LIGHT_0662_fits__*pix.png resample_wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20_00sec_-15_00C_LIGHT_0153_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: 2461033.00158644 23.12.2025 12:02:07.068 /data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits
First image: 2461033.00158644 23.12.2025 12:02:07.068 /data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits
Last image: 2461121.79708253 22.03.2026 07:07:37.931 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 11
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.45
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 7895
Objects passed selection criteria: 7892
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 7684.5
Average stars matched: 7471.5 (97.2282 %)
Memory usage VmPeak: 113712 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Mar 22 02:31:50 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: 2461033.00158644 23.12.2025 12:02:07.068 /data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits
First image: 2461033.00158644 23.12.2025 12:02:07.068 /data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits
Last image: 2461121.79708253 22.03.2026 07:07:37.931 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 38
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.22
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: 13 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): 39842
Objects passed selection criteria: 39738
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 39122.5
Average stars matched: 37667 (96.2796 %)
Memory usage VmPeak: 140572 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Mar 22 02:32:38 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/TTUQ1b1x1/TTUQ1_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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits
SExtractor catalog cache: saved Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits.cat to cache
SExtractor catalog cache: saved Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.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/Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.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: 2461121.79626927
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_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits exists and is non-empty
Saving wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits to local_wcs_cache/
'wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits' -> 'local_wcs_cache/wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits'
wcs_Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits exists and is non-empty
Saving wcs_Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits to local_wcs_cache/
'wcs_Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits' -> 'local_wcs_cache/wcs_Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits'
wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits exists and is non-empty
Saving wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits to local_wcs_cache/
'wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits' -> 'local_wcs_cache/wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits'
wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits exists and is non-empty
Saving wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits to local_wcs_cache/
'wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits' -> 'local_wcs_cache/wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 10:00:00.529 +30:00:00.78
Second-epoch image center 10:00:00.178 +29:59:57.72
Angular distance between the image centers 0.00 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 10:00:00.529 +30:00:00.78
Second-epoch image center 10:00:03.099 +30:00:38.14
Angular distance between the image centers 0.01 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 10:00:00.178 +29:59:57.72
Second-epoch second image center 10:00:03.099 +30:00:38.14
Angular distance between the image centers 0.01540 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/Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits &> /tmp/tmp.k04r2X625u
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits &> /tmp/tmp.GUOmiAbTtF
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits &> /tmp/tmp.2fHKLOLWhv
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits &> /tmp/tmp.uR5oRNCC6v
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.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_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits and wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.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_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits and wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits.cat
Found non-empty wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits and wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits.cat
The reference image (wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits) and catalog (wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits.cat) found
'wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.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 4292 out of 7639 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.950909
a=0.000000 b=1.000000 c=22.950909
From vast_summary.log: estimated ref. image limiting mag.: -7.45
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.50
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.50
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 11 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits
2.1 pix Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits
2.1 pix fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits
2.1 pix fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits
Limiting magnitude estimates:
15.5 mag. Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits
15.5 mag. Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits
15.5 mag. fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits
15.5 mag. fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits
All-image limiting magnitude estimate: 15.5 (SNR ) 12.4 (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.k04r2X625u (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_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits' -> 'wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits
WCS_IMAGE_NAME=wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits
WCS-calibrated image found: wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits
Checking if the catalog wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits.cat corresponding to the image wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits alredy exist and is non-empty...
Catalog wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits.cat corresponding to the image wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits
WCS catalog name: wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=548, passed=7639
Got 7639 stars (including 7079 good ones) from the SExtractor catalog wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits.cat
util/solve_plate_with_UCAC5 got 7639 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 916 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: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
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 916 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.31"
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 916 stars left (next iteration limit 1007)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits -region wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.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.GUOmiAbTtF (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_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits' -> 'wcs_Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits
WCS_IMAGE_NAME=wcs_Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits
WCS-calibrated image found: wcs_Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits
Checking if the catalog wcs_Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits.cat corresponding to the image wcs_Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits alredy exist and is non-empty...
Catalog wcs_Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits.cat corresponding to the image wcs_Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits
WCS catalog name: wcs_Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=575, passed=7653
Got 7653 stars (including 7069 good ones) from the SExtractor catalog wcs_Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits.cat
util/solve_plate_with_UCAC5 got 7653 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 917 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 917 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 917 stars left (next iteration limit 1008)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits -region wcs_Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.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.2fHKLOLWhv (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_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.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_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits
WCS_IMAGE_NAME=wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits
WCS-calibrated image found: wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits
Checking if the catalog wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits.cat corresponding to the image wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits.cat corresponding to the image wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits
WCS catalog name: wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=500, passed=7830
Got 7830 stars (including 7321 good ones) from the SExtractor catalog wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits.cat
util/solve_plate_with_UCAC5 got 7830 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 912 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: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.26"
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 912 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.26"
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 912 stars left (next iteration limit 1003)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits -region wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.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.uR5oRNCC6v (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_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.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_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits
WCS_IMAGE_NAME=wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits
WCS-calibrated image found: wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits
Checking if the catalog wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits.cat corresponding to the image wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits.cat corresponding to the image wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits
WCS catalog name: wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=525, passed=7832
Got 7832 stars (including 7288 good ones) from the SExtractor catalog wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits.cat
util/solve_plate_with_UCAC5 got 7832 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 914 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: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.28"
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 914 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.27"
Estimated accuracy of the plate solution: 0.26"
Excluding outliers - 914 stars left (next iteration limit 1005)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits -region wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.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_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits'
Saving fully-calibrated image wcs_Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/wcs_Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits'
Saving fully-calibrated image wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits'
Saving fully-calibrated image wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits'
Preparing the HTML report for the field Leo-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20413.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20426.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20428.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out20414.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 20413_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154
The candidate 20413_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154 did not pass the final checks
**** FOUND 09:46:12.90 +29:34:54.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)GAIADR2_OUTPUT=# 0.312 648447294697816960 146.55369540152 +29.58178851744 12.4267 12.0195 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.312#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20414_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154
Preparing report for the candidate 20414_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20417_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154
The candidate 20417_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154 did not pass the final checks
**** FOUND 09:25:17.15 +29:58:47.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20420_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154
The candidate 20420_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154 did not pass the final checks
**** FOUND 10:26:31.23 +34:18:36.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20423_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154
The candidate 20423_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154 did not pass the final checks
**** FOUND 10:06:05.07 +30:50:49.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20424_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154
The candidate 20424_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154 did not pass the final checks
**** FOUND 10:23:41.63 +29:53:37.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20425_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154
The candidate 20425_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154 did not pass the final checks
**** FOUND 10:22:28.53 +33:00:39.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20426_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154
The candidate 20426_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154 did not pass the final checks
**** FOUND 10:04:44.24 +31:33:26.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 0.530 745736412850483584 151.18438749198 +31.55708252860 12.5147 12.2304 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.530#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20427_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154
The candidate 20427_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154 did not pass the final checks
**** FOUND 10:07:32.44 +28:23:04.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20428_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154
The candidate 20428_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154 did not pass the final checks
**** FOUND 09:56:24.94 +28:51:55.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 0.108 743523366526266624 149.10392918753 +28.86533316719 12.4174 11.9478 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.108#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06133_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154
The candidate 06133_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154 did not pass the final checks
**** FOUND 10:02:40.95 +26:41:37.0 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 6s
Prepared the HTML report for the field Leo-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
10:34:36.19 +28:41:52.3
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits
SExtractor catalog cache: saved Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits.cat to cache
SExtractor catalog cache: saved Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits /data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits
Creating symlink local_wcs_cache/wcs_Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits
Creating symlink local_wcs_cache/wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.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_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits exists and is non-empty
wcs_Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits exists and is non-empty
wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits exists and is non-empty
wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 10:00:00.529 +30:00:00.78
Second-epoch image center 10:00:00.178 +29:59:57.72
Angular distance between the image centers 0.00 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 10:00:00.529 +30:00:00.78
Second-epoch image center 10:00:03.099 +30:00:38.14
Angular distance between the image centers 0.01 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 10:00:00.178 +29:59:57.72
Second-epoch second image center 10:00:03.099 +30:00:38.14
Angular distance between the image centers 0.01540 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/Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits &> /tmp/tmp.kXbti4lwgJ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits &> /tmp/tmp.3OSLsz5ahX
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits &> /tmp/tmp.04LOM2HJwc
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits &> /tmp/tmp.7jBj53bdJ5
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits
Calibrating the magnitude scale
Found non-empty wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.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_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits and wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.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_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits and wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits.cat
Found non-empty wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits and wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits.cat
The reference image (wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits) and catalog (wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits.cat) found
'wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.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 4346 out of 39721 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.850684
a=0.000000 b=1.000000 c=22.850684
From vast_summary.log: estimated ref. image limiting mag.: -7.22
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.63
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.63
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 24 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits
1.9 pix Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits
2.1 pix fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits
2.1 pix fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits
Limiting magnitude estimates:
15.6 mag. Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits
15.6 mag. Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits
15.6 mag. fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits
15.6 mag. fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits
All-image limiting magnitude estimate: 15.6 (SNR ) 14.9 (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.kXbti4lwgJ (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_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits' -> 'wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits
WCS_IMAGE_NAME=wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits
WCS-calibrated image found: wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits
Checking if the catalog wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits.cat corresponding to the image wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits alredy exist and is non-empty...
Catalog wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits.cat corresponding to the image wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits
WCS catalog name: wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=1754, passed=39706
Got 39706 stars (including 37890 good ones) from the SExtractor catalog wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits.cat
util/solve_plate_with_UCAC5 got 39706 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 911 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 911 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 911 stars left (next iteration limit 1002)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits -region wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.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.3OSLsz5ahX (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_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits' -> 'wcs_Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits
WCS_IMAGE_NAME=wcs_Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits
WCS-calibrated image found: wcs_Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits
Checking if the catalog wcs_Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits.cat corresponding to the image wcs_Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits alredy exist and is non-empty...
Catalog wcs_Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits.cat corresponding to the image wcs_Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits
WCS catalog name: wcs_Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=1766, passed=39901
Got 39901 stars (including 38068 good ones) from the SExtractor catalog wcs_Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits.cat
util/solve_plate_with_UCAC5 got 39901 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 910 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
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 910 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: 0.33"
Excluding outliers - 910 stars left (next iteration limit 1001)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits -region wcs_Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.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.04LOM2HJwc (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_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.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_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits
WCS_IMAGE_NAME=wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits
WCS-calibrated image found: wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits
Checking if the catalog wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits.cat corresponding to the image wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits.cat corresponding to the image wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits
WCS catalog name: wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=1498, passed=38753
Got 38753 stars (including 37200 good ones) from the SExtractor catalog wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits.cat
util/solve_plate_with_UCAC5 got 38753 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 908 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: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.28"
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 908 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.28"
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 908 stars left (next iteration limit 998)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits -region wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.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.7jBj53bdJ5 (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_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.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_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits
WCS_IMAGE_NAME=wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits
WCS-calibrated image found: wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits
Checking if the catalog wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits.cat corresponding to the image wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits alredy exist and is non-empty...
Catalog wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits.cat corresponding to the image wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits
WCS catalog name: wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=1596, passed=39050
Got 39050 stars (including 37389 good ones) from the SExtractor catalog wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits.cat
util/solve_plate_with_UCAC5 got 39050 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 910 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: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
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 910 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.30"
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 910 stars left (next iteration limit 1001)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits -region wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.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_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.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_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/wcs_Leo-01-Q1b1x1_2025-12-23_06-02-07_20.00sec_-15.00C_LIGHT_0662.fits
Saving fully-calibrated image wcs_Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.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_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/wcs_Leo-01-Q1b1x1_2025-12-23_06-02-45_20.00sec_-15.00C_LIGHT_0663.fits
Saving fully-calibrated image wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.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_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-06-27_20.00sec_-15.00C_LIGHT_0153.fits
Saving fully-calibrated image wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.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_2026-03-22_CI_Leo-01-Q1b1x1_020826_TTUQ1b1x1_31619_k53KPIzP/wcs_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154.fits
Preparing the HTML report for the field Leo-01-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out52830.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52833.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52834.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52836.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53140.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53209.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53210.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53228.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53267.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53284.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53354.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53358.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out53232.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out52936.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52987.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 52830_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154
The candidate 52830_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154 did not pass the final checks
**** FOUND 09:33:24.68 +31:05:01.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.65, MAG_FAINT_SEARCH_LIMIT=15.63)
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Considering the candidate 52833_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154
The candidate 52833_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154 did not pass the final checks
**** FOUND 10:26:55.21 +33:27:04.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.61, MAG_FAINT_SEARCH_LIMIT=15.59)GAIADR2_OUTPUT=# 1.728 749191971738527616 156.72958213086 +33.45093326298 14.4335 13.9103 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.728#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52834_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154
The candidate 52834_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154 did not pass the final checks
**** FOUND 10:24:06.55 +34:03:10.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.77, MAG_FAINT_SEARCH_LIMIT=15.75)GAIADR2_OUTPUT=# 2.944 749282921965930368 156.02648688939 +34.05235994347 15.3150 14.7637 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.944#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52836_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154
The candidate 52836_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154 did not pass the final checks
**** FOUND 10:33:48.36 +31:10:49.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 0.908 747778240302926848 158.45126401080 +31.18018233718 14.0343 13.4744 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.908#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52841_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154
The candidate 52841_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154 did not pass the final checks
**** FOUND 10:34:36.19 +28:41:52.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 52936_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154
Preparing report for the candidate 52936_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154
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Considering the candidate 52937_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154
The candidate 52937_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154 did not pass the final checks
**** FOUND 09:48:36.16 +33:25:17.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52987_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154
Preparing report for the candidate 52987_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154
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Considering the candidate 53012_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154
The candidate 53012_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154 did not pass the final checks
**** FOUND 10:05:00.42 +29:44:35.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53091_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154
The candidate 53091_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154 did not pass the final checks
**** FOUND 09:40:34.05 +28:22:40.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53102_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154
The candidate 53102_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154 did not pass the final checks
**** FOUND 09:50:53.15 +31:21:43.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53140_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154
The candidate 53140_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154 did not pass the final checks
**** FOUND 09:33:29.57 +32:45:37.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.58, MAG_FAINT_SEARCH_LIMIT=15.56)GAIADR2_OUTPUT=# 1.975 701059853801380608 143.37372620157 +32.76019422687 14.5582 14.0355 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.975#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53193_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154
The candidate 53193_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154 did not pass the final checks
**** FOUND 09:37:32.01 +32:12:59.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53209_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154
The candidate 53209_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154 did not pass the final checks
**** FOUND 10:30:38.37 +24:32:24.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.96, MAG_FAINT_SEARCH_LIMIT=15.94)GAIADR2_OUTPUT=# 2.457 724324351612529152 157.65928217007 +24.53974844168 15.1519 14.6310 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.457#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53210_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154
The candidate 53210_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154 did not pass the final checks
**** FOUND 10:09:32.70 +30:58:19.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.91, MAG_FAINT_SEARCH_LIMIT=15.89)GAIADR2_OUTPUT=# 3.808 745505785991419648 152.38580661420 +30.97115182564 15.3594 14.9024 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.808#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53228_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154
The candidate 53228_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154 did not pass the final checks
**** FOUND 09:33:57.33 +26:17:52.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.97, MAG_FAINT_SEARCH_LIMIT=15.95)GAIADR2_OUTPUT=# 0.648 646140553662490496 143.48906342947 +26.29771543288 15.0978 14.5962 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.648#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53232_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154
The candidate 53232_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154 did not pass the final checks
**** FOUND 09:28:06.30 +26:23:00.3 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.74, MAG_FAINT_SEARCH_LIMIT=15.72)
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Considering the candidate 53266_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154
The candidate 53266_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154 did not pass the final checks
**** FOUND 09:51:48.96 +34:07:24.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53267_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154
The candidate 53267_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154 did not pass the final checks
**** FOUND 10:32:23.12 +29:51:30.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.97, MAG_FAINT_SEARCH_LIMIT=15.95)GAIADR2_OUTPUT=# 1.306 735526828911487360 158.09623881334 +29.85890883954 14.8671 14.3666 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.306#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53284_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154
The candidate 53284_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154 did not pass the final checks
**** FOUND 09:59:11.02 +28:18:54.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.98, MAG_FAINT_SEARCH_LIMIT=15.96)GAIADR2_OUTPUT=# 1.417 743249450692091904 149.79551784947 +28.31498849893 15.1333 14.6120 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.417#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53354_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154
The candidate 53354_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154 did not pass the final checks
**** FOUND 09:28:26.23 +32:56:35.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.92, MAG_FAINT_SEARCH_LIMIT=15.90)GAIADR2_OUTPUT=# 1.906 701297588830984832 142.10869062978 +32.94306136960 14.9705 14.3462 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.906#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53358_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154
The candidate 53358_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154 did not pass the final checks
**** FOUND 09:30:29.41 +26:55:29.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.99, MAG_FAINT_SEARCH_LIMIT=15.97)GAIADR2_OUTPUT=# 0.644 694278959433108864 142.62263722013 +26.92478713798 14.8272 14.2795 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.644#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 19485_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154
The candidate 19485_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154 did not pass the final checks
**** FOUND 09:25:17.16 +29:58:47.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33041_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154
The candidate 33041_fd_Leo-01-Q1b1x1_2026-03-22_02-07-37_20.00sec_-14.90C_LIGHT_0154 did not pass the final checks